Contents

Contents

The Pennsylvania State University · The Graduate School · Department of Electrical Engineering · 1985

Beam Steerable Microwave Antenna
for Automotive Radar Application

Suggested citation — McGinn, Vincent Paul. Beam Steerable Microwave Antenna for Automotive Radar Application. Ph.D. dissertation, The Pennsylvania State University, 1985.

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BEAM STEERABLE MICROWAVE ANTENNA FOR AUTOMOTIVE RADAR APPLICATION

Vincent Paul McGinn

1985

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The Pennsylvania State University

The Graduate School

Department of Electrical Engineering

Beam Steerable Microwave Antenna for Automotive Radar Application

A Thesis in

Electrical Engineering

by

Vincent Paul McGinn

Submitted in Partial Fulfillment of the Requirements for the Degree of

Doctor of Philosophy

May 1985

© 1985 by Vincent Paul McGinn

I grant The Pennsylvania State University the nonexclusive right to use this work for the University’s own purposes and to make single copies of the work available to the public on a not-for-profit basis if copies are not otherwise available.

(signed) Vincent Paul McGinn

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We approve the thesis of Vincent Paul McGinn.

Date of Signature:

  • 28 Feb 85Dale M. Grimes, Professor of Electrical Engineering and Head of the Department, Committee Chairman and Thesis Advisor
  • 7 March 85Lynn A. Carpenter, Associate Professor of Electrical Engineering
  • 28 Feb 85Leslie E. Cross, Professor of Electrical Engineering
  • 28 Feb 85Peter D. Usher, Associate Professor of Astronomy
  • 28 Feb 85Francis T. S. Yu, Professor of Electrical Engineering
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ABSTRACT

Research described herein reports on the techniques developed for documenting the performance of an experimental (baseline) forward looking collision avoidance automotive radar system. The system studied operates at a frequency of 36 Gigahertz and emits a beam stationary with respect to the vehicle. On-the-road testing has been accomplished and deficiencies are highlighted. Specifically, “false alarms” caused by highway guard rails and complex traffic situations are demonstrated in an 18-minute television production suitable for public broadcasting. The program utilizes panoramic views of actual driving situations accompanied by real time telemetry data representing vehicle dynamics and radar system response. Data gathered suggests performance enhancement (lower false alarm rate and improved resolution) through the use of a beam steerable antenna. Since the ultimate goal of perfecting an automotive collision avoidance radar system should be widespread consumer application, cost effectiveness is a necessity. To this end, a new microwave device and technique are suggested. Cadmium Selenide (CdSe) is proposed as a photoconductive material suitable for Apparent Geometry Modification (AGM) of a low power radiating structure. A primitive microwave antenna which incorporates the photoconductive device has been constructed and analyzed. Test results have matched design expectations completely.

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TABLE OF CONTENTS

Page
ABSTRACT iii
LIST OF CHARTS viii
ACKNOWLEDGEMENTS ix

CHAPTER

  1. INTRODUCTION — 1
    • 1.1 Automotive Radar Potential — 1
    • 1.2 Automotive Radar Practicality — 3
    • 1.3 Objectives of this Work — 6
  2. BACKGROUND — 11
    • 2.1 Research Vehicles Description — 11
      • 2.1.1 Warning Decision — 12
      • 2.1.2 Radar Sensor Description — 14
      • 2.1.3 Radar Sensor Traits — 17
    • 2.2 Performance Data Documentation — 18
      • 2.2.1 Telemetry System Considerations — 19
        • 2.2.1.1 Telemetry Transmitter — 22
        • 2.2.1.2 Telemetry Receiver — 27
        • 2.2.1.3 Telemetry System Calibration — 29
      • 2.2.2 Completed Television Production — 30
  3. PROBLEM STATEMENT — 37
    • 3.1 Beam Steering Techniques — 37
    • 3.2 Apparent Geometry Modification (AGM) — 42
    • 3.3 Apparent Geometry Modification (AGM) Stimulation — 44
  4. MICROWAVE PHOTOCONDUCTORS — 49
    • 4.1 Material Characteristics — 49
      • 4.1.1 Resistance — 52
      • 4.1.2 Light History — 53
      • 4.1.3 Speed of Response — 55
      • 4.1.4 Spectral Response — 58
    • 4.2 Device Configuration — 59
      • 4.2.1 Fabrication — 63
    • 4.3 Device Characterization — 64
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Table of Contents, continued

CHAPTER

  • 4.3.1 Intrinsic Capacitance Determination — 65
  • 4.3.2 Inductance Determination — 70
  • 4.3.3 Tuning to Desired Frequency of Response — 75
  • 4.4 Test Fixture Characteristics — 79
  1. RADIATING STRUCTURE DEMONSTRATION — 83
    • 5.1 Bihorn Array — 83
      • 5.1.1 Bihorn Characteristics — 86
    • 5.2 Demonstration Equipment — 88
    • 5.3 System Performance — 92
      • 5.3.1 Predicted Performance — 93
      • 5.3.2 Observed Performance — 94
  2. CONCLUSION — 99
    • 6.1 Summary Remarks — 99
    • 6.2 Recommendations for Further Research — 101

REFERENCES — 105

Appendix Page
I Phase Plane with Warning Boundary 114
II Block Diagram of Radar Sensor 116
III Range Calibration for Ford Granada 118
IV Data Documentation Technique 120
V Telemetry Signals 122
VI Telemetry Transmitter Schematics 125
VII Telemetry Receiver Schematics 130
VIII Telemetry Calibrator 136
IX Microstrip Fed Horn Antenna Suitable for AGM 138
X Unloaded Horn 140
XI Loaded Horn 142
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Table of Contents, continued

Appendix Page
XII Semiconductor Energy Diagram 144
XIII Type 4, CdSe Typical Resistance vs. Illumination Characteristics 146
XIV Variation of Conductance with Light History 148
XV Minimum Search Time Determination (RF Considerations) 150
XVI Type 4, CdSe Peak Spectral Response 690.0 Nanometers 154
XVII LED Optical Output Characteristic 156
XVIII LED Transfer Characteristic 158
XIX Equivalent Microwave Circuits 160
XX Microwave Photoconductive Element 162
XXI Microwave Photoconductive Element Models 164
XXII Geometric Model used in Determining Total (Untuned) Device Capacitance 166
XXIII Total Device Capacitance Calculations 168
XXIV Microwave Photoconductive Element with Tuner 171
XXV SMA Test Fixture Performance 173
XXVI Mini Pharaoh Radiation Pattern 178
XXVII Isotropic Sources Spaced 3λ/2 180
XXVIII Bihorn Radiation Pattern 182
XXIX Antenna RF Configuration 184
XXX Schematic Diagram of Microwave Transmitter 186
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Table of Contents, continued

Appendix Page
XXXI Bihorn Phasor Calculations (Amplitude to Phase Conversion) 189
XXXII Inductance Formula Sensitivity Analysis 192
XXXIII Demonstration Equipment Photographs 199
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LIST OF CHARTS

Chart Page
1 Information Transmission Methods 20
2 Fourier Components Attenuation 25
3 Steering Techniques 42
4 Type 4 Cadmium Selenide Response Times 56
5 Observed Beam Steering 96
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ACKNOWLEDGEMENTS

A fortunate individual prospers from motivation offered by caring parents during early stages of development. I am thankful to both of my parents for the encouragement they provided to expand and enhance my technical talents and interests. Good fortune also accompanied me with a truly excellent research committee. I wish to thank Dr. Dale Grimes for suggesting the original thesis topic and for providing guidance in the areas of automotive radar and electromagnetics. I am also thankful to Dr. Lynn Carpenter, Dr. L. Eric Cross, Dr. Peter Usher, and Dr. Francis Yu for the expert advice they made available in the areas of microwave techniques, materials, data analysis, and electro-optics, respectively.

I am grateful to the following agencies and industries for providing financial support: U.S. Department of Transportation (NHTSA), U.S. Veterans Administration, RCA Inc., Harris Corporation, and Proctor and Gamble. The technological support provided by Data Display Products and muRata Erie North America Inc. is also appreciated.

I am especially indebted to Mr. Norman Wolff and Vactec Inc. Through their generosity with photoconductors the central theme of this dissertation was realized.

Penn State staff personnel provided much assistance during various project phases. I particularly wish to recognize the efforts of Mr. William Burkhard, Mr. Anthony

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Cingle, Mr. Vernon Eminhizer, Mr. John McClelland, Mr. Joseph Stewart, and Mr. Carl Volz, Jr.

Numerous fellow students and colleagues devoted time and effort in support of this dissertation. Much gratitude is due to Dr. Thomas Baginski, Mr. Kenneth Carroll, Dr. William Fleming, Mr. Juan Muci, and Mr. Russ Taras.

I wish to thank Dr. Anthony Ferraro for his comments and recommendations regarding antennas. His empathy and friendship is continually appreciated.

Mr. Al Valeski provided outstanding drafting. The manuscript was professionally typed by Mrs. Debbie Putt. Both of these individuals merit special commendation. Their responsiveness was appreciated many times.

Dr. Richard Duckworth instilled in me the initial confidence to undertake a program of advanced study at Penn State. His support is deeply appreciated.

It must be said that novel research demands much of a spouse. Mary Sue provided more than understanding. She provided support and dedication. She deserves the special “thank you” for helping me past the trying moments.

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CHAPTER 1

INTRODUCTION

1.1 Automotive Radar Potential

Each year thousands of people lose their lives in automotive mishaps. Even more people sustain debilitating injury ranging from dislocations to limb loss. On 30 December 1984, Columbia Broadcasting, by way of its popular television program, “Sixty Minutes,” extolled the virtues of automotive air bags in saving lives and preventing serious injury. In support of safety devices (like air bags), statistics are often quoted. In a year’s time, over 45,000 lives will contribute to the American highway fatality statistic [8]. Of course, to believe that a single safety device or even a multitude of safety options could eradicate fatality (and serious injury) statistics entirely is foolhardy. Yet, there exists a class of accidents which does not have to be as violent and as injurious as they are [14]. Further, there is yet a class of accidents which may be entirely avoided. Consider the late-night situation where the unthinking operator is “over-driving” the headlamps: Illumination does not cover a sufficient distance for a safe panic stop. If, let us say, there was a stalled second vehicle on the road without warning lights, a

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collision is highly probable. If the road is curved or if the weather is less than optimum, the probability of a mishap is further increased. It is clear in such a case that the accident may be avoided entirely if warning of the obstruction (target) is provided to the driver in sufficient time to react. Even the most conscientious driver would welcome advance warning of an impending hazard. This is the basis for a forward looking collision avoidance radar system. One should not, however, regard such a radar system as a panacea for avoiding all classes of impacts. A situation may be posed, for example, where the physical dynamics dictate that a collision must occur. Yet the severity of numerous collisions could be lessened by the operator responding just an instant quicker. Thus, a forward looking collision avoidance radar system could provide accident mitigation. Besides providing timely operator warning, other possibilities associated with the application of automotive radar become apparent: passive restraint system sensitivity control and “smart” cruise controls. As a safety system, however, automotive radar must be regarded as separate from all others. Other safety measures (like seat belts or air bags) presume the accident has already taken place and attempt to protect the vehicle’s occupants during the impact. In contrast, radar is deployed with the intent of avoiding the impact in advance. Some investigations have suggested the possibility of an

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automatic radar controlled brake [50]. It is not difficult to imagine, however, how this over-ambitious application of radar could create more problems than it solves! Product liability is an area that technologists cannot ignore. The experimental work conducted during the initial phase of the presented research involved vehicles that are capable of automatic antiskid braking as prompted by a signal from the forward looking radar if a limit beyond the operator warning limit (light and tone provided) is exceeded. These experimental systems, therefore, have been referred to as: “Collision Avoidance Radar Braking Systems” [105], or “Radar Brakes.” At no time, however, were the vehicles operated on the road with this automatic feature engaged. To take (even a portion of) control away from the operator may result in unexpected and quite deleterious results. It is indeed difficult to imagine that such an automatic brake would ever be practical or even desirable!

1.2 Automotive Radar Practicality

The development of a practical consumer oriented automotive collision avoidance radar system just 20 years ago was unthinkable. This is not at all surprising since two needed techniques were immature at that time: low-cost, reliable microwave components and the necessary signal processing electronics. However, in the past 10 years, this nation has witnessed a phenomenal growth in radio frequency

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(RF) communications products and small-scale electronic data processing equipment. To emphasize the profundity of this statement, consider each area separately: First, realize that X-band (10.5 Gigahertz) doppler radar transceivers are replacing door mat switches for activation of automatic doors at supermarkets, airports, and hospitals. It is indeed difficult to imagine that a cost effective and reliable replacement has been made for the simple mat switch! The RF components used in these doppler radar transceivers are not unlike the “front end” of an automotive radar system. Commercially available RF sources are presently available up through the millimeter wavelengths (100 GHz) [35]. Millimeter wavelengths are especially attractive in terms of package miniaturization. Gallium Arsenide and Indium Phosphide Gunn sources are capable of meeting the modest output power (20 milliwatts) requirements for automotive radar. Second, consider that a basic four-function, hand-held calculator with no memory sold for approximately $200 just 15 years ago. The same instrument can be had today for just under five dollars. Microprocessors today are seen everywhere. The 8 and 16 bit personal microcomputers are currently in vogue, with the possibility of a 32 (and higher) bit machine for the home on the horizon. Microprocessors and associated firmware have become so economical that their strengths are being exploited in a spectrum of consumer products including

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sewing machines, food blenders, and washing machines. Many persons who have witnessed the impressive performance of the experimental vehicles studied in this research are surprised to learn that the warning decision computation is performed by a basic 8 bit microprocessor (INTEL 8080, NMOS). Since, of course, these experimental vehicles do not have spatial microwave beam scanning capability, the processing being accomplished only embraces kinematic calculations. However, with the aid of high density, inexpensive electronic data storage techniques, microwave beam scanning could provide target signature (pattern) recognition.

State-of-the-art memory technology is represented by random access memories (RAMs) with 256 kilobits per chip. Fujitsu Ltd. has demonstrated a 256 kilobit dynamic RAM with access times below 100 nanoseconds. With gate lengths of only 2.5 microns, the entire chip occupies an area of 34.1 square millimeters. One million bits on a single chip should make its debut this year [35].

It should be recognized that solid state technologies for the production of digital and RF devices are not mutually exclusive. In fact, microstrip and finline techniques are entirely feasible at frequencies beyond 100 Gigahertz [64, 81]. Thus, many digital device production methods (like masking and photolithography) are directly applicable to the manufacture of RF circuitry and components. This single observation explains why production

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costs in both areas are plummeting. An additional benefit to be derived for automotive radar capitalizes on the possibility of an integrated system on a single substrate. This may appear quite ambitious at the present stage of development. However, economical and reliable automotive radar sensors would follow from volume requirements. From a technological standpoint, there is presently no reason why such an integrated assembly is not practical. The sensor would incorporate a beam scanned planar antenna, duplexer, microwave generator (source), modulator, control electronics (supervisory and signal coding to eliminate interunit interference), amplification, and detection. The entire unit would be placed directly in back of the rear view mirror of the vehicle. This area allows for an unobstructed high outlook position for the radar beam. This location also poses no ambient stresses beyond those that other sophisticated automotive electronic systems (e.g., electronic fuel injection and spark control) endure. The proposed radar sensor would be no larger than the rear view mirror itself.

1.3 Objectives of this Work

This work is a contributory effort to advance forward looking collision avoidance automotive radar systems from developmental stages closer to a consumer product. Three significant research phases are presented: First, the

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technique developed for documenting the performance of an experimental (baseline) automotive collision avoidance radar braking system is described. An 18-minute television production suitable for public broadcasting is the culmination of this exploratory phase. Depicted within the program are actual over-the-road driving situations (panoramic views) with associated real time telemetry (radar processor signals reflecting electronic system response and vehicle dynamics). The television program (interview format) is tutorial by nature. Yet, it adequately demonstrates the impressive performance of an automotive radar system utilizing technology which is almost a decade old. The program also highlights the deficiencies caused by an emitted beam which is not spatially steered with respect to the vehicle. Specifically, “false alarms” caused by highway guard rails and complex traffic situations are demonstrated. These false (or nuisance) alarms would hamper widespread deployment and acceptance of forward looking collision avoidance automotive radar systems simply because of confidence degradation by the vehicle operator. Therefore, the second phase of this research was conceived to explore the possibility of developing an inexpensive (but reliable) electronic means of achieving spatial beam scanning.

If such an effort could be achieved, numerous possibilities for reducing the false alarm rate become

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practical. Beam steering, which follows the driver’s steering angle, immediately comes to mind. A more powerful technique entails continuous scanning. This would allow for target signature (pattern) recognition of impending hazards. This would invoke digital signal storage and processing methods which are already available.

After much examination of previous antenna beam steering techniques, it was realized that none were suitable for the automotive radar application and the frequencies of interest (10 Gigahertz through 100 Gigahertz). The departure from established techniques was necessitated in order to meet reproducibility, reliability, and cost requirements in the harsh ambient environment imposed by automotive vehicles. A practical solution was sought. To this end, it was necessary to conceptualize antennas in their most basic form. Electromagnetic radiators may consist of only two components: electrical conductors and electrical insulators (dielectrics). If it would be possible to vary the electrical conductivity of the structure at electronic speeds the consequence would be apparent geometry modification (AGM) of the structure with the attendant positioning of the emitted beam. A computer simulation has been performed verifying this theory is correct. Crucial to the success of such a technique is obviously the availability of a suitable material. More generally, a universal device which could be applied to most

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any structure would be highly desirable. The control (modulating) signal should be supplied to the variable conductivity material without resorting to an electrical connection. This “action at a distance” would allow for total decoupling (isolation) of the radio frequency (RF) components from the controlling input. A photoconductive compound became the obvious choice for material. In this research, Cadmium Selenide (CdSe) was used with total success at a frequency of 10.5 Gigahertz. Use of this material at the frequencies of interest was heretofore unknown. Even at lower frequencies, substrate capacitive reactance masks photoconductivity variations. Success is achieved through planar (monolithic) minimal capacitance topology with inductive tuning. By careful application of lumped element (LE) techniques, it is entirely feasible to achieve wideband (Q less than 20) electrical resonance. Conductivity modulation of the device at and around resonance mimics direct current performance. The planar configuration of the fabricated microwave photoconductive element yields a device which is not multimodal. A clearly defined (and repeatable) single resonance is exhibited. These devices can also be used to provide variable attenuation along a microstrip signal path. By judicious choice of electrical circuit configuration it is possible to achieve amplitude variation to phase variation conversion. Thus, the microwave photoconductive elements

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may be applied to existing conformal phased arrays obviating the need for new structure development. Embedded in phase three of this research is a demonstration of the application of the microwave photoconductive device. Beam steering is accomplished for a rudimentary monopole bihorn radiating structure. Both microstrip fed horn patches are operated against a ground plane. In spite of relatively low forward gain (17.0 decibels), up to 10.0 degrees of beam steering may easily be observed. Only two microwave photoconductive devices are used to feed the structure. The steering command signal is supplied to the chips via Gallium Aluminum Arsenide (GaAlAs) light emitting diodes (LEDs). The spectral peaks of the illumination supplied by these optical emitters (660 nanometers) is extremely close to the peak of the Cadmium Selenide optical spectrum (690 nanometers).

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CHAPTER 2

BACKGROUND

2.1 Research Vehicles’ Description

The Electrical Engineering Department at The Pennsylvania State University has been fortunate to have on loan from the U.S. Department of Transportation, National Highway Traffic Safety Administration, two vehicles incorporating collision avoidance radar braking systems. These vehicles were made available for independent engineering analysis from 1980 through 1985. During this time, many hundreds of hours of over-the-road driving data and impressions were accumulated. Both vehicles were modified by the Bendix Corporation Research Laboratories in Southfield, Michigan, 48076, at a total contract cost of $400,000. The vehicles represent a full-size (1977 Plymouth Fury) sedan and a mid-size (1977 Ford Granada) sedan. Although both vehicles incorporate antiskid braking subsystems, research described herein concerns itself only with the forward looking radar system.

The radar system consists of three major subassemblies: the antenna and associated RF microwave components (the front end), the radar (video) electronics module, and the signal processor console (computer, control, and display).

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The radar sensor provides estimates of closure rate and range to a target. These estimates are supplied as inputs to an 8 bit microprocessor-based digital computer. The computer continuously processes these signals along with other inputs representing signal presence, vehicle velocity, and various inhibit functions (driver input commands, such as: steering angle, driver braking, and mode of system operation). In the subsections which follow, the basic warning decision technique will be discussed first, followed by a description of the radar sensor which supplies critical information to the digital processor.

2.1.1 Warning Decision

Numerous algorithms may be formulated to determine when to alert the driver of an impending mishap. However, consider the physics of a typical situation: Kinetic energy (K.E.) increases as the square of the velocity (v) of a vehicle with respect to a reference point (stationary or moving). That is:

where m = vehicle mass. The stopping distance (x) may be defined as that distance which is required to bring the vehicle in close proximity to the target (without actually contacting the target) with a relative velocity of zero at the time of osculation. If one assumes a constant

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decelerating force (F) on the vehicle, we note:

but,

where a is a constant deceleration. Therefore:

or

or

where k is a constant based upon deceleration; or

where is the first derivative of x with respect to time.

The implication of this analysis results in a phase plane boundary. Refer to Appendix I. If the range (x) is plotted versus range rate () assuming a constant deceleration (here 0.7 G) we note that a parabolic curve is developed. If 0.7 G is the maximum attainable deceleration, it is recognized that operation of the vehicle to the right of the phase plane boundary will result in an impact. Thus,

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to the left of the phase plane boundary are drawn two piecewise linear boundaries: The one on the extreme left represents a warning limit. If the operator crosses this boundary (from left to right), the system renders a visual (light) and aural (beeper) warning. If the second boundary is crossed (left to right), the radar system sends a command to the antiskid automatic braking system. The boundaries are stored as permanent memory in the computer. Where the vehicle is operating with respect to these boundaries is determined by digital processing.

2.1.2 Radar Sensor Description

⚠️ [The original prints this heading as “2.1.1”; renumbered to 2.1.2 to match the Table of Contents.]

The sensor is comprised of a radome, antenna, doppler transceiver, and a separate electronics module. The radome provides protection from the elements. The antenna is an eight inch parabolic dish mounted in a central opening of the vehicle’s grille. Frequency of operation is at 36.0 Gigahertz. The antenna achieves horizontal and vertical half power beamwidths of about 3.1 degrees. Although circular polarization would undoubtedly be a better choice,1 linear polarization is employed with a 45 degree cant to the horizontal. This provides approximately 20 decibels of suppression of “blinding” from a similarly equipped vehicle. The high gain antenna with low sidelobe levels also aids in

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significantly reducing the probability of car-to-car blinding.

The doppler transceiver develops a peak pulse power of approximately 25.0 milliwatts at 36.0 Gigahertz. It is of the Gunn effect variety (Gallium Arsenide) and provides self-detection (homodyning) of the reflected echo signals.

See Appendix II for a block diagram of the radar sensor. The electronics module provides the transceiver with the necessary pulse modulation. ON-OFF pulse modulation results in a positive range cutoff feature. Modulation is accomplished as follows:

  1. RF output at 36 GHz + 410 kHz for 730 ns.
  2. No RF output for 1420 ns.
  3. RF output at 36 GHz − 410 kHz for 730 ns.
  4. No RF output for 1420 ns.
  5. Cycle repeats.

Within the transceiver, reflected echoes are combined with samples of the transmitted RF energy in the circulator. Homodyne detection occurs in the mixer. The resultant doppler difference signal (video) is amplified in the preamplifier before further processing. The video output, of course, is pulsed and similar to the RF output. At this point, however, it is appropriate to regard these high frequency detected pulses as a “carrier” for the lower frequency doppler modulating component. Only the last 215 nanoseconds of these pulses is gated alternately into the

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two amplifier/limiter chains. The sampled data after filtering and further amplification becomes a reconstruction of continuous doppler target information in each of the two channels. Range rate information is recovered as a frequency (doppler) to voltage conversion from one channel only (the range rate detector). Electrical phase comparison between the signals from each channel provides range information (the range detector). The sense of velocity, approach or recede, is accomplished by noting the electrical phase (lead or lag) of the signals between the channels. The threshold channel rejects targets which are too weak (amplitude), or at too low relative velocity. Range rate and range outputs from radar sensor are of an analog (direct current voltage) nature. See Appendix III for typical range calibration data. Ideally, a linear correlation between the data and voltage is desirable. This, in practice of course, is seldom seen. Displacement error () is therefore defined [67]:

where - = actual output voltage - = voltage which would occur for a linear relationship - = full scale (upper limit) voltage.

For this definition, it must be realized that the ideal linear relationship (a line) intersects the end points of

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the actual curve. Therefore, represents the largest vertical departure of the actual curve from the ideal relationship. The radar sensor outputs exhibit typical displacement errors on the order of 7.5%. Actual vehicle speed information is derived from magnetic sensor/toothed wheel combinations placed on the front wheels and rear axle differentials of the vehicles. Displacement error is slightly better for the direct measurement devices than for the radar sensor.

2.1.3 Radar Sensor Traits

Since the transmitter is chirping at two frequencies separated by 820 kilohertz, range determination becomes ambiguous for targets beyond 300 feet. However, restricting the transmitted pulses to 730 nanoseconds duration eliminates responses from targets at ranges beyond 250 feet. This has been confirmed theoretically and experimentally [25].

This radar system possesses no inherent range resolution of separate targets. Because of the limiters in each channel, outputs of the sensor represent the target producing the strongest return signal. In principle, therefore, it would be possible for a large target far away to mask a smaller target which is much closer to the vehicle. This close-in invisible target problem could be

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alleviated by spatially steering the emitted beam of RF energy.

2.2 Performance Data Documentation

Numerous drivers were enlisted to evaluate the performance of the experimental vehicles. However, well-meant but ambiguous qualitative reports pointed up the need for a data documentation technique. As initially conceived, the panoramic view of the driving scenario was considered to be of highest importance. With the current availability of reliable, compact video cameras and recorders (VTR) documenting the performance of an automotive collision avoidance radar system reduces to eliminating mechanical vibrations imparted to the TV camera under normal operating conditions and developing a convenient means of simultaneously recording numerical data which represents input and output signals to and from the radar control computer. The first problem is easily solved by a mechanical low pass filter which mounts the video camera inside the vehicle. This “filter” is nothing more than a flat board cushioned with polyurethane foam and secured with compliant rubber straps. The second problem is solved with the aid of a telemetry system which simultaneously records numerical data on the audio channel of the video system as the panaromic view is being transcribed on the video channel. Thus, at the time of playback with a videotape

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player (VTP), audio is routed to a telemetry receiver for decoding and display of said data. Refer to Appendix IV for a block diagram of the data documentation technique. At the time of data analysis, actual over-the-road driving situations are replayed as a television display along with the following decoded parameters: vehicle speed, range, closure rate, and warning (light and beeper). With the aid of a studio switcher and a television camera (trained on the data display), a split screen display is generated. On the top of the screen is displayed system operating parameters. Immediately below this display is the panoramic view of the driving situation. These composite driving sequences are then edited for incorporation into the final production: “Automotive Radar, A Technical Review and Analysis,” The Pennsylvania State University, Quad Master #11-1007.

2.2.1 Telemetry System Considerations

In recording data electronically, two decisions are necessary: First, should the format be digital or analog? Second, should the modulation be linear (amplitude) or non-linear (angle)? Angle modulation may be accomplished by frequency or phase variations [10, 102, 107]. In terms of the required resolution (e.g., Speed − 1 km/hr), each channel would require a minimum capacity of 7 bits [57]. Based upon the fact that the data to be recorded is already in analog format and the available audio frequency (AF)

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voice channel is inherently designed to handle continuously varying (amplitude) information with low distortion. quantification required for a digital system offers no advantage [57]. Furthermore, bandwidth limitations on the AF channel must be taken into account with regards to the maximum sampling frequency. When system complexity and cost effectiveness are added as primary considerations, analog format is the preferred technique of information transmission. Angle modulation is inherently wideband. While phase locked loops (PLL) may be used in signal demodulation, aliasing or harmonic locking can be a serious problem [10, 41, 107]. Improper “locking” also rules out the possibility of a fail safe system. Our format/modulation choice is therefore Analog/AM. This is a narrowband, fail safe technique. See Chart 1.

Chart 1 — Information Transmission Methods

Possible Formats Possible Modulations
1. Digital 1. Amplitude (AM)
2. Analog 2. Angle (Frequency or Phase)

Method Selected: Analog/AM

To minimize cross talk between telemetry channels, the following system design parameters have been accounted for:

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  1. The signalling frequencies are not harmonically related. (See Appendix V for telemetry output signals and interface specifications.)
  2. The individual channel signals must be low in distortion content.
  3. The receiver filters must be very selective frequency wise (high Q with sharp skirts).

In the telemetry system, better than 39 decibels (dB) isolation between channels has been achieved. High Q filters require excellent long-term stability. Because of stability considerations, active filters must be ruled out in the receiver [30]. Digital (switched capacitor) filters would be acceptable within the receiver except for complexity [31]. A novel filtering scheme for decoding the telemetry revolves around an electromechanical filter manufactured by Erie muRata Manufacturing Co. [65]. These filters are miniature tuning forks with piezoelectric transducers attached to the tines. Narrow, reproducible bandpass characteristics are realized with these filters. The high stability and low cost of these so called “Microforks” made them an obvious choice for the telemetry receiver design. The only precaution to observe in the Microfork application has to do with their susceptibility to mechanical vibration. This deficiency was sidestepped by acoustically isolating the circuit boards on which the filters are attached from the chassis with vinyl grommets.

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The Microforks proved to be excellent filters for our application. The telemetry system operation is straightforward. The next three subsections describe telemetry system components: the transmitter, the receiver, and the calibrator.

2.2.1.1 Telemetry Transmitter

Refer to Appendix VI for complete schematic diagrams of the telemetry transmitter. The “Input Isolation and Signal Conditioning (DC) Amplifier” consists of two dual operational amplifiers (LM 747 CN). Analog DC signals from the radar processor are first impedance buffered (1.0 megohm) by U1A, U2A, and U2B. Attenuation (X0.46) and offset (as provided by 5.0 kilohm potentiometers in voltage divider configurations) are introduced at this point so that the modulators (transistors Q1) are operated over the most linear portion of their characteristic (+0.4 to +2.6 Volts collector supply). The outputs of U1A, U2A, and U2B (speed, closure rate, and range) feed an inverting unity gain direct coupled amplifier (U1B). The output from this amplifier feeds the slave/alarm channel. Thus, if the output on U1A or U2A or U2B should rise (or lower), then the output of U1B will lower (or rise) by an equal amount. The slave channel audio signal is ultimately combined with the other channels’ audio signals so that a constant composite telemetry signal is made available to the television

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camera’s audio input. The RCA Color Video Camera Model CC 007 used in this research incorporates an automatic gain control (AGC) on its audio channel. Amplitude modulation would therefore be ineffective except that the slave channel reproduces a signal which is a negative differential of variations which are occurring on the speed, closure rate, and range channels. Since AGC action depends on either peak or average (not RMS!) rectified values of composite waveforms, the slave channel prevents the AGC from interfering with the modulation process. A side benefit derived from the AGC, however, has to do with self-regulation of the composite waveform eliminating the need for a regulated power source at the telemetry transmitter! Low pass single section RC filters consisting of 10.0 kilohm resistors and 2.2 microfarad capacitors are inserted at the outputs of U1A, U1B, U2A, and U2B in order to suppress possible switching transients and noise.

The Input Isolation and Signal Conditioning Amplifiers derive their power from the radar system. This is the only portion of the transmitter requiring external power. This choice was made for the DC amplifiers to minimize drift that would otherwise be caused by relative shifts between different power sources. The remainder of the transmitter utilizes complementary metal oxide semiconductors (CMOS) in both digital and linear configurations [13, 63]. A nine volt power source consisting of six 1.5 volt primary

p. 24

Alkaline Magnanese-Dioxide cells, No. 335 (ANSI “L 70”) in series proves to be entirely adequate for the application. The transmitter with an LED pilot lamp only draws approximately 38 milliamperes at the stated voltage. The Alkaline Manganese-Dioxide system was selected over the more conventional LeClanche batteries because of their graceful degradation of voltage with use and longer life [24].

The “Precision AF Signal Generation” for all four channels is similar and will be discussed simultaneously. Specified within Appendix V are quartz crystal frequencies, counter divide ratios, resistor and capacitor values (, , and ). The high Q filters employed in the receiver require excellent frequency stability of the transmitter AF signals. To this end, high frequency quartz crystal controlled oscillators (U3A, MC 14007AL) provide high stability signals to CMOS frequency dividers (U4, MC 14040AL binary counters). The crystals are accurate to ±0.01% over the intended operating temperatures. At the highest AF signal frequency (1050 Hz) this corresponds to a variation of only 0.1 Hz. After frequency division, the resultant square wave is amplitude modulated by a bipolar transistor (Q1 in each channel). With appropriate gain proportionment embedded within the AC coupled amplifiers (U3B and U3C, MC 14007AL), the square wave’s higher order Fourier harmonics are suppressed by a three stage () low pass filter (LPF). Recognizing that the square wave harmonics fall off

p. 25

at a rate of −6.0 dB/octave [42] and that the low pass filter is providing an additional −18.0 dB/octave rolloff, a calculation of the harmonic components after filtering is possible. See Chart 2.

Chart 2 — Fourier Components Attenuation

Frequency Octave Relative Amplitude Octave (−24 dB)
—– 0 dB
1.585 −38 dB
2.322 −55.7 dB
2.807 −67.4 dB
etc. etc. etc.

[Note: the fourth row is printed “” in the original though it denotes the 7th harmonic (7f) — an apparent typo for .]

It is seen that the sinusoids are indeed quite low in residual distortion [42, 85]. The three stage RC low pass filter is of passive design. At the AF operating (fundamental) frequencies, the amplitude transmission factor for these three stage networks is quite low (1/10π). However, they have the most desirable feature of low Q. Low Q assures swift response time with no ringing. Audio output levels from each U3B amplifier is individually adjustable by a linear taper 100 kilohm potentiometer.

The warning signal provided by the overall radar system is of an ON/OFF nature. A telemetry channel similar to the ones provided for speed range and rate of closure could then

p. 26

be used for warning signalling. However, this would be a poor choice since dynamic range for the other channels would have to be reduced. A far better method used here exploits the benefits of frequency shift keying (FSK). Within Appendix VI, refer to “FSK and Output Summer.” Since the frequency of the slave channel is of little consequence we may shift its frequency depending on the absence or presence of a radar warning signal. Detection is elementary since a Microfork filter may be selected to have its resonant frequency correspond with one of the slave channel frequencies (warning condition). Notice that twice 378 Hz and twice 389 Hz make for symmetrical harmonics about 767 Hz eliminating the possibility of false readings on the closure rate channel if nonlinearities are present in the overall system and a warning signal is being transmitted. FSK is simply accomplished by electronically switching crystals (387,072 Hz and 398,336 Hz) via two silicon steering diodes (1N4148). Forward or reverse alternate bias to the diodes is achieved by switching transistor Q2. The FSK section of the transmitter produces an 11 Hz output deviation. All AF telemetry signals are mixed by a low pass passive summer. The output signal from the summer is injected directly into the video camera audio input.

p. 27

2.2.1.2 Telemetry Receiver

The telemetry receiver is of straightforward design. Refer to Appendix VII for complete schematic diagrams of the receiver. The composite audio signal is impressed at the “Input Amplifier.” This section provides a 600 ohm input impedance, adjustable voltage gain, and signal distribution to the Microforks. A voltage divider residing at the output of U1 (LM 741CN operational amplifier) assures safe, acceptable signal levels to the Microforks. The Microforks in each “Channel Amplifier” require input and output terminations of 300 kilohms. These terminations are accomplished by a passive signal distribution network at the output of the Input Amplifier and impedance buffers (AC coupled operational amplifiers) at the inputs of the Channel Amplifiers. The Channel Amplifiers for speed, range, and closure rate function are similar. At the input of each Channel Amplifier appears the Microfork filter (MF1) and associated impedance buffer (U2A, 1/2 section LM 747CN dual operational amplifier). The impedance buffer has a gain of 6.6 dB. Further amplification is provided by U2B with a gain of 27.5 dB. Both U2A and U2B are AC coupled. It should be mentioned that all operational amplifiers throughout the system, whether DC or AC coupled, are biased for minimum drift due to temperature variations [66]. The output signal from U2B is detected via a half wave voltage doubling rectifier circuit incorporating germanium diodes

p. 28

(1N270). At this point it is only necessary to restore proper DC levels (offset) and provide appropriate DC amplification. The former is accomplished with a 10 kilohm potentiometer fed from the ±12 VDC supply rails. The offset voltage is added to the detected signal at the inverting input of U3A (1/2 section LM 747CN dual operational amplifier). This stage actually produces no voltage gain (÷−2.0 for speed and range function). For the closure rate channel, a selectable voltage division ratio of this stage is made available (÷−2.0 or ÷−1.2). Thus, two display ranges for closure rate (50.0 m/sec or 30.0 m/sec, respectively) are possible. Following U3A the signal is amplified by U3B. This stage affords adjustable DC gain (X−1.2 to X−6.2). Individual channels are calibrated by adjusting DC gains and offsets. This offers the advantage over AC gain adjustment in that the two adjustments (zero and full scale) do not interact. In the event of signal loss, the meters are protected by germanium (1N270) reverse catching diodes. The overall system rise time would be limited by the response time of the Microforks (100 msec. typical); however, further damping (480 msec.) is introduced in order to cause the indicators to mimic automotive speedometer behavior. Actually, critical damping has been accomplished and the response time is one third the limit imposed on speedometers by SAE standards [90]. Analog instrumentation (microammeters) was selected over "seven

p. 29

segment" displays because an analog presentation depicts trends with no further mental interpretation required.

The Channel Amplifier for the Warning Alarm within the receiver is identical to other Channel Amplifiers up to the output of the half wave voltage doubling rectifier. Here, the detected signal is routed to the inverting input of U4 (LM 741CN, single operational amplifier) which provides a voltage gain of 2.15. The output signal of U4 is passed through a single section RC low pass filter (LPF). The LPF is a measure against false triggering. The output signal from the LPF is applied to the noninverting input of U5 (LM 311N voltage comparator). The inverting input is biased at −8.0 volts from a resistive voltage divider fed from positive and negative power supply rails. The switched output of this comparator controls an incandescent lamp (1819) and a solid state audible alarm (Sonalert SC 628). The lamp filament is biased to be warm with no visible emission continuously by a 1.8 kilohm resistor. This insures long bulb life and a crisp turn warning characteristic. The telemetry receiver is entirely self-contained and is powered from an internal power supply operated from the AC mains.

2.2.1.3 Telemetry System Calibrator

Two point calibration of the telemetry system is accomplished via an accessory calibrator which uses two

p. 30

Alkaline Manganese-Dioxide batteries, cell designation No. 315 (ANSI “L40”) [24]. This results in a telemetry system linearity of better than 1.0% displacement error. Periodic checks with a laboratory digital voltmeter verified (test jacks provided on calibrator) cell potential. Additionally, provision for exciting the FSK (warning channel) portion of the transmitter is made. This guarantees proper operation of the entire telemetry system. Refer to Appendix VIII for a schematic diagram of the calibrator. The calibrator is used at the beginning and end of each data gathering session by electrically patching it to the telemetry system inputs.

2.2.2 Completed Television Product

The telemetry system described in previous subsections indeed proved to be the key to successful data documentation. Many hours of video tape footage were gathered under actual vehicle operation. Even more time was expended in reviewing the recorded information. As one might expect, much duplication of events was noted. It was possible, however, to extract situations which represented both normal and anomalous events. Nearly all of the documented happenings were spontaneous and unanticipated. A few staged situations were recorded to demonstrate certain system characteristics which might otherwise go unnoticed. Eleven individual segments were selected for incorporation into the final television production. This show (18

p. 31

minutes) features Dr. Dale M. Grimes as interviewed by Mr. Frank Wilson. “Automotive Radar, A Technical Review and Analysis” is aimed at a general audience. The interview itself serves as a tutorial for the uninitiated. The show is also of interest to technologists since it highlights the problems requiring resolution in quantitative terms. Thus, it is possible to describe the 11 segments and their intended purposes:

Clip 1. This depicts unremarkable rural two-lane driving with oncoming traffic. The road curves to the right. Guard rails abound on-coming traffic. The radar system performs in a normal fashion with no warning provided. Range and closure rates are noted to vary continuously with captured targets.

Clip 2. The research vehicle approaches the rear end of a tractor trailer truck at a moderately high speed (70.0 kilometers/hour). The truck has pulled out into the lane in which the radar equipped car is travelling. The target is acquired at a range of 45.0 meters. A warning is rendered at a closure rate of 9.0 meters/second. A second warning is issued as the driver passes in the left lane. The second warning is a consequence of the high rate of closure on the median guard rail.

p. 32

Clip 3. A five-lane, in-town road is depicted (two lanes going, two lanes coming, and one center turn lane). The research vehicle is travelling on the outermost lane (adjacent to turn lane). A second vehicle exiting from a bank crosses out over the first lane into the second lane and is now travelling in the same direction as the research vehicle. Of course, the second vehicle is at a much lower speed and blocks the research vehicle’s path. The research vehicle is travelling at 55.0 kilometers/hour. The target is acquired at a range of 18.0 meters. A warning is rendered at a closure rate of 6.0 meters/second.

Clip 4. This segment demonstrates changing lanes at highway speeds (90.0 kilometers/hour). The research vehicle changes from the left lane to the right lane on a four-lane highway (with center divider). A target in the right lane is acquired. The range is 35.0 meters. With a 0.0 meters/second closure rate, no warning is elicited.

Clip 5. The research vehicle is travelling at a moderately high speed (70.0 kilometers/hour). The driver is negotiating a turn in the highway. The radar acquires a metal guard rail as a valid target

p. 33

(erroneously) at a range of 30.0 meters. The angled closure rate is noted to be 15.0 meters/second. The radar system renders a “nuisance” warning. This clip demonstrates the most important problem hampering large-scale deployment of automotive radar as a consumer product: “the false alarm.”

Clip 6. Around town slow-speed driving is demonstrated. Pulling up too quickly (delayed braking) on the rear of a stopped vehicle renders a valid warning response from the radar system. The research vehicle is initially travelling at 20.0 kilometers/hour. At a range of 11.0 meters, the target is noted. The warning alarm is provided at a closure rate of 3.0 meters/second. This clip also demonstrates how the radar system is calibrated such that the zero point for range is slightly in front of the radar antenna. That is, zero range actually occurs approximately 1.5 meters in front of the radar antenna. Of course, any “cushion” is possible. As the vehicle ahead pulls away, a dip in range is observed back to zero. Beyond the 1.5 meter cushion, normal range calculations are resumed.

p. 34

Clip 7. The research vehicle is deliberately being driven at an abnormally high speed through a parking lot. Numerous alarms are rendered because the radar system is being operated above the low speed cut off. Vehicle speed is observed to vary between 10.0 and 20.0 kilometers/hour. Range varies between 5.0 and 10.0 meters. Typical closure rates are approximately 3.0 meters/second.

Clip 8. A bicyclist is stopped at a four-way intersection. The research vehicle cautiously approaches from the rear at 5.0 kilometers/hour. The final range with the research vehicle stopped is observed to be 2.0 to 3.0 meters. The closure rate is too low to be observed. No warning is rendered. The range dramatically increases as the bicyclist pulls away. The radar clearly has captured the target. The research vehicle then turns into the intersection. The range fluctuates as a building is intercepted by the radar beam.

Clip 9. The research vehicle is stopped at an intersection with the radar operating in a normal fashion. As pedestrians, cars, bicycles, and trucks pass in front of the radar beam system response is noted. The range fluctuates as target interception takes

p. 35

place. The narrowness of the emitted beam may be clearly observed (~3.1 degrees).

Clip 10. The research vehicle is travelling through a parking lot at a nominal speed of 10.0 kilometers/hour. A lady pushing a baby carriage crosses the path of travel. The range is noted to be 15.0 meters. A warning is rendered by the radar system. The event is of short duration with low (unregistered) closure rate.

Clip 11. This final segment is referred to as a basic complex traffic situation. The vehicle is approaching a red light in the right lane. The road curves to the right before the intersection. Vehicles are stopped in the left lane awaiting a left turn signal. The research vehicle’s initial speed is observed to be 25.0 kilometers/hour. The radar beam intercepts the stopped vehicles. At a range of 15.0 meters target capture occurs. A false alarm warning is rendered at a closure rate of 4.5 meters/second. The research driver is negotiating a normal turn and is braking in an acceptable fashion. Yet, the radar system is “fooled” by the tangential velocity component reflected from the parked vehicles.

p. 36

In the 11 clips just outlined, an array of most important driving encounters is represented. Other situations could, of course, be envisioned. However, after examining many other encounters, similarities were noted. The 11 clips are by no means all inclusive. They do represent a fair depiction of many like situations. The most important result is contained in video tape footage depicting the false alarm phenomenon. A consumer product must be believable. False alarms reduce operator confidence. The system must not distract the operator unnecessarily. Therefore, system integrity enhancement must embrace a solution to the false alarm. The solution to the problem resides in processing and/or microwave beam steering. The highest dividends reside in the latter area. The fact that this statement is correct resides in the observation that beam steering produces more information to be processed. In other words, the most advanced algorithm renders little performance improvement with sparse system inputs. Therefore, the central goal of the presented research focuses on an inexpensive means of microwave beam steering.

p. 37

CHAPTER 3

PROBLEM STATEMENT

3.1 Beam Steering Techniques

The methods by which an emitted radio frequency (RF) beam may be steered are shown in Chart 3. To select a suitable technique for automotive radar, one must keep in mind cost and reliability. Both concerns are critical. First, the antenna must not drive the cost of the entire system. Second, the antenna is most prominent in determining overall system performance. The antenna characteristics must be reproducible and predictable. No other system component can compensate for an erratic antenna. Thus, a mechanically steered antenna is ruled out of consideration immediately. It would be costly because of tight mechanical tolerance requirements. It would be physically large and inherently unreliable in the harsh automotive environment. Interest is therefore focused only on non-mechanical techniques. A discussion of each non-mechanical method is provided:

Phased arrays have found widespread application for long-range radar systems and commercial communications [16, 44, 48, 49, 52, 84, 92]. The technique employs many individual radiators where the phase/amplitude of the

p. 38

electrical signal driving each radiator is altered with relation to other radiators. This allows for beam steering at electronic speeds. From a pure geometric analysis of the technique, the effects are easily understood. The obvious drawbacks of the system embrace cost and complexity. Although the system of radiating elements may be fabricated without difficulty, the problem of realizing a suitable phase/amplitude controller presents a major concern. At high power levels ferrite phase shifters [37] are commonly exploited to achieve the required excitation alterations. These devices are quite large and expensive. They certainly do not lend themselves to monolithic fabrication techniques due to the required large magnetic bias. For low power levels, PIN diodes have been used as signal controllers with good success [4, 37]. The PIN diode suffers from two drawbacks: Junction capacitance limits the useful upper frequency limit and the control signal (bias) is electrically connected to the device itself. The latter deficiency presents a serious concern relative to isolating the bias from the RF signal path.

Synthetic prisms have been used for electromagnetic beam steering. A fairly well known method [61] relies on an intricate system of waveguides with apertures so arranged that when the frequency of the excitation is shifted the phase relationship of waves emitted from each aperture is altered. Thus, beam steering is achieved from frequency to

p. 39

phase (time lag) conversion. This system must immediately be discarded for automotive radar because of its inherent wide band nature. A more modern approach to the synthetic prism is affected from shining monochromatic radiation through a crystal at a non-orthogonal angle. It is well known that the square root of the ratio of dielectric constants of different materials is related to the linear ratio of refractive indices [80]. Thus, beam steering may be achieved by modulating either the frequency [17] of excitation or the dielectric constant of one material (a ferroelectric) [56]. The latter suggestion is the focus of much commercial interest and most information about the subject is of a proprietary nature [15]. Modulation of the dielectric constant of a ferroelectric material may be accomplished by controlling an applied DC electrostatic field along the crystal. The technique is currently hampered by several pitfalls: a) the static field required is quite high (10 kilovolts/cm), b) polycrystalline forms of the material are very lossy at microwave frequencies due to scattering and absorption, c) single crystals are high in cost, and d) the crystal’s environment causes unwanted secondary steering.

Anisotropy modification in various forms may be utilized to achieve electromagnetic beam steering. The possibility of constructing a single radiator (not an array) with the capability of beam steering is indeed an exciting

p. 40

endeavor. At least one team of investigators [71] has successfully integrated ferrite materials into a biconical radiator. Beam steering is accomplished by varying static magnetic fields. The technique is satisfactory up through L band. For X band and beyond, high static magnetic fields are not only difficult to confine, but also present geometric interference with the electromagnetic radiator itself. This particular area, however, suggests strong promise and may ultimately be attractive up through the millimeter wavelengths. Anisotropy modification may also be accomplished with a plasma [26]. For many years, synthetic dielectrics (dielectrics supporting embedded conductors) have come into being. A plasma may be viewed as a synthetic dielectric in this respect. It should be obvious then that altering the ion population (ensemble or local) could achieve electromagnetic wave steering. For automotive radar it is difficult, however, to envisage this technique in a practical light. Maintenance of the plasma at specified ionization levels for extended periods of time would be most difficult, indeed.

Rectilinear beam positioning to angular conversion is a well established electromagnetic beam steering technique used in ground aviation applications for height finder radars. The basis of operation may be explained with the aid of geometry [92, 95]. Parabolic reflectors are normally illuminated at the focus and emitted rays from the reflector

p. 41

are parallel. However, if a parabolic torus is illuminated off focus but normal to the directrix, the reflected ray passes through the focus at some angle with respect to the directrix. If the illumination is moved towards or away from the focus, while maintaining a right angle with the directrix, the new ray still passes through the focus but achieves a different angle with respect to the directrix. Clearly, then, to steer the beam requires nothing more than separate radiators with excitation which may be switched on or off. Suitable switches in low power applications make use of solid state diodes [37]. At extremely high frequencies, low junction capacitive reactance must be taken into account. Switching times between 20 and 600 nanoseconds are not uncommon. Variability amongst diodes presents a significant manufacturing (selection and matching) problem.

Apparent Geometry Modification (AGM) was ultimately considered as the preferred method to achieve electromagnetic beam steering for automotive radar. Sparse information on the subject area is available. Yet, recent developments in materials are about to cause considerable interest in this previously unnoticed area. Although research presented herein concerns itself with photoconductive compounds, other investigators (Japan) are presently studying Apparent Geometry Modification via “conductive plastics.” Certain conductive plastics exhibit

p. 42

variable local conductivity characteristics with respect to applied mechanical stress. It is understandable that nearly all information on the fabrication and application of these materials is proprietary [1]. The concept of Apparent Geometry Modification is profound but easily understood. The technique is described separately in the next section.

Chart 3 — Steering Techniques

  1. Mechanical
  2. Phased Arrays — (Ferrite Phase Shifters Commonly Employed)
  3. Synthetic Prism —
      1. Frequency Variation
      1. Dielectric Constant Variation
  4. Anisotropy Modification
  5. Rectilinear Beam Positioning to Angular Conversion
  6. Apparent Geometry Modification

3.2 Apparent Geometry Modification

Apparent Geometry Modification (AGM) is a new and relatively unexplored method for accomplishing electromagnetic beam steering. While geometry modification of antennas has been reported [7], the alterations were of a mechanical nature. Recognizing that a radiating structure consists of electrical conductors, dielectrics, or both, it would appear reasonable that beam position and shape could

p. 43

be modified by varying conductivity. This may be regarded as changing the conductive material’s geometry. Suitable materials for such application would capitalize on a bulk effect. Photoconductive materials such as Cadmium Sulfide (CdS), Cadmium Selenide (CdSe), Zinc Sulfide (ZnS), and Zinc Selenide (ZnSe) are in this category [21, 56]. Photoconductors have been employed before at microwave frequencies. Sun, Cheng, and Walsh [93] have reported the use of microwaves to bias a photoconductor consisting of mercury doped germanium. No one to date has considered using a photoconductive material as part of an antenna system. This should not be surprising for two reasons: a) For transmitting, resistance introduced into the structure destroys efficiency [44]. b) For receiving, resistance introduced into the structure produces noise [51]. However, in automotive radar applications, efficiencies as low as 10 or 20% mean dissipating powers on the order of only 40 milliwatts. Also, the return signals to the system are so strong that homodyne detection is all that is required. The signal to noise ratio remains good by virtue of the strong return signal. Apparent Geometry Modification should not be regarded as a panacea for beam positioning. A low power situation probably represents the only suitable application of a material which can vary conductivity in a continuous manner. It should be recognized, however, that photoconductors do offer some unique features. Unlike

p. 44

semiconductor junctions which are small and isolated, a photoconductor can occupy a significant portion of the antenna’s area. Continuous beam steering along with continuous beam shaping is therefore possible. Also, light which would be the controlling signal can easily be confined, focused, and accurately distributed.

3.3 Apparent Geometry Modification (AGM) Simulation

Before actually constructing an antenna which incorporates a photoconductive compound in the structure, it is reasonable to perform a simulation in order to predict the radiator’s performance. On file at The Pennsylvania State University is an Antenna Modelling Program (AMP) [3]. Any surface may be modelled with a finite element grid. This finite element model (FEM) is entirely satisfactory if the grid cells are kept small [68, 92]. Recommendations for segment length [1, 68, 92] place an upper limit of approximately 0.1 wavelength. For grids selected to be analyzed, segments were added and deleted while maintaining a maximum limit on cell size. No alterations were observed in radiated patterns. This technique confirms that the grid used in the investigation is satisfactory and the recommendations regarding segment length are correct. The AMP has a maximum computational limit of 500 segments. The structure examined has 466 segments. In selecting an antenna for analysis, a practical but elementary structure

p. 45

is desirable. The selected geometry represents a wire fed horn. This is an excellent candidate since in actual practice, microstrip [36, 38, 103] would be used to feed a conformal array [70].

A 3-to-4 relative geometric ratio for the grid cell was established. See Appendix IX. This was necessary in order to secure integral grid connection points. Data is available on wire fed pyramidal horns that use equilateral triangles on all sides [72]. The departure for the model from the equilateral case is not severe (67.38 degrees, 56.31 degrees, 56.31 degrees). The triangle is first developed in the XY plane. The leading edge is 2.0 wavelengths long. The height is 1.5 wavelengths long. In order to establish a perfect imaginary pyramid (with the image reflected in the XY ground plane), it is necessary to rotate the structure about the Y axis by 41.81 degrees:

AMP has this rotational capability. Single point voltage feed is utilized. Ultimately, experiments will be performed at X band. The computer simulation was carried out at 300 Megahertz for the reason that one meter equals one wavelength at this frequency. Thus, all geometric tabulations were easily read in terms of wavelength directly. Since perfect conductivity for the grid and ground plane is specified, no inconsistency in scaling

p. 46

results [92]. The developed structure is 100% efficient with a maximum gain of 13.33 dB at an azimuthal (phi) angle equal to 180 degrees. As expected, at this angle the wave is linearly polarized in the vertical direction. See Appendix X. In the next simulation, segments were loaded with resistance simulating the photoconductive material. A slot is “cut” in the structure where the material will be inserted. To determine a suitable place to make the cut, the following reasoning is used: From the channel (cut) to the feed point, a smaller horn is established. The difference in forward gains between the total horn and this smaller horn will be called “differential gain.” If the cut is made close to the feed, the slot controls large differential gain but has little effect on the off-center steering angle. On the other hand, if the cut is made close to the leading edge, a wide steering angle is possible with little differential gain control. The mathematical product of geometric steering angle and differential gain is formed. The first derivative of this product with respect to geometric steering angle is calculated. This derivative is set equal to zero. Thus, the optimum geometric steering angle (without regard to current distribution) is found to be 55.81 degrees off center. In terms of the flat surface forming the upper side of the horn, the cut should be made at −0.9331 wavelengths away from and running parallel to the Y axis. The actual loading segments occur between −0.975

p. 47

and −0.9 wavelengths. See Appendix IX. The affected segments are labelled “J through X.” In series with segment “J” is inserted a 288 kilohm resistance. Segments “K through S” are series loaded with individual resistance values of 240 kilohms. Segments “T through W” have individual series resistance values of 750 ohms inserted. The final segment “X” is loaded with a 900 ohm series element. All other geometric and electrical parameters remain unchanged from the previous case. All resistances selected for this simulation represent typical values which can be achieved in a most reliable manner with Cadmium Selenide material. The radiation pattern for this loaded horn is displayed in Appendix XI. A slight loss in efficiency (91.36%) was noted in the simulation. The beam shape has been radically altered with the appearance of a back lobe. The important observation to be made, however, is that the maximum gain (12.12 dB) is attained off center (185 degrees). Of course, the steering effect would be more pronounced with an array. An important area of research would center on the development of an optimization of individual radiator size versus array size to achieve the desired steering, gain, beamwidth, and sidelobe levels. A conformal array could be developed which possibly would include a dielectric lens or reflector [18, 47, 49, 52, 53, 68, 70, 99]. Parasitic coupling is also a concern which must be accounted for in the inherent design of an array.

p. 48

Classical analysis techniques coupled with data processing methods may be invoked for these considerations [27, 48, 49, 73, 98]. Travelling wave antennas [101] may be excellent candidates for Apparent Geometry Modification and the application of photoconductive elements.

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CHAPTER 4

MICROWAVE PHOTOCONDUCTORS

4.1 Material Characteristics

Photoconductivity is a bulk material phenomenon which is characterized by reduced electrical resistivity across a semiconductor because of impinging optical radiation of the proper frequency. Electrical current may flow in either direction since no PN junction is involved. The effect has been known for many years [21]. To understand its origin it is convenient to examine a form of Ohm’s Law:

where - = current density - = conductivity - = applied electric field

The conductivity in a semiconductor may be represented as follows:

where - = electron concentration - = electron mobility - = hole concentration - = hole mobility - = particle (electron) charge

p. 50

Conductivity may therefore be increased by elevating particle mobility or making more carriers available. In the case of photoconductivity, this latter mechanism is achieved through broken covalent bonds. It is convenient to refer to an energy diagram for the material. See Appendix XII. Three types of particle transitions may be secured from optical excitation: a) a photon may excite a donor electron with energy into the conduction band, b) a photon may excite a valence electron into an acceptor state with a final excited energy of , and c) electron-hole pairs may be created by high energy photons. The first two transitions are referred to as impurity excitation. The last transition is known as an intrinsic excitation.

Electron-hole pairs are produced at a rate of . The carriers will exhibit a statistically distributed lifetime of (mean). This lifetime is not unlike current injected carriers (as in a transistor). Steady state carrier density may now be defined:

This is a special case of the solution to the more general continuity equation for excited carriers. Thus, conductivity increases due to the increased number of mobile holes and electrons:

p. 51

Commercial photoconductors exhibit much larger conductivity excursions (for a given optical energy deviation) beyond what this equation predicts. This is a consequence of “trapping” [21]. Trapping essentially hinders normal recombination. If one type of carrier is easily trapped, the other type remains in its conduction band. Recognizing that this phenomenon contributes significantly to conductivity variations, it is possible to formulate a new equation accounting for excess electrons:

where = concentration of excess electrons

Trapped carriers exhibit a mean lifetime which is much longer than . The effects of traps may be expressed in terms of an effective quantum yield Y [21]. This is a measure of the number of electrons passing through external connections to the device per photon absorbed in the sensitive region. If Y is less than unity, the photocurrents are known as primary. If Y is greater than unity, the photocurrents are referred to as secondary. For commercial Cadmium Selenide (CdSe) and Cadmium Sulfide (CdS) photoconductors, the quantum yield is between 100 and 10,000. This indicates the important role of trapping in such devices. During the experimental phases of this research Cadmium Selenide was selected as the most promising candidate for investigation. This choice was a consequence

p. 52

of low ON (saturated) resistance, wide dynamic resistance range, low hysterisis, and rapid speed of response.

4.1.1 Resistance

Cadmium Selenide (CdSe) used in this project was supplied by a commercial manufacturer of photoconductive cells (Vactec, Inc., St. Louis, Missouri, 63132). Electrical resistance measurements were made on sample devices for three levels of illumination: a) total darkness, b) 2.0 foot candles, and c) 100.0 foot candles. The equivalent resistivity for each of these cases corresponds approximately to ohms/square, ohms/square, and ohms/square, respectively. The accompanying resistance for individual devices of course is dependent upon the geometry of exposed photoconductive compound (the channel). The channel is formed by the space which appears between the ohmic contacts (normally Indium). Thus, for uniform but otherwise equivalent levels of optical radiation, it is noted that a narrow channel produces low electrical resistance. In addition, if the total linear length of the channel is increased, the electrical resistance may be further reduced. For example, refer to Appendix XIII. A family of curves is plotted for different devices. Curve “D” is typical of the performance of Vactec’s VT-241H. Curve “E” represents the performance of part number VT-241. Both of these devices

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are just 0.15 inches at the widest diameter. Types VT-14L and VT-34L performance is represented by curve “G.” The first device is approximately 0.35 inches at the widest diameter, while the second is approximately 0.26 inches across the widest diameter. All devices utilize an alumina () substrate of 0.040 inch thickness. Curve “C” in Appendix XIII represents the equivalent performance of the experimental microwave devices. These devices (curve “C”) were fabricated with the intention of incorporating them into an actual beam steerable microwave antenna.

The Cadmium Selenide employed in this research is referred to as “Type 4” by the trade. Although Cadmium Sulfide is more popular in industrial applications, Cadmium Selenide was specified for research purposes because of the low ON resistivity. In all cases, experimental test data for the devices exceeded minimum performance specifications supplied by the manufacturer.

4.1.2 Light History

The general discussion of material characteristics (section 4.1) suggests that photoconductors should exhibit hysterisis with regard to conductance. This material “memory” or “fatigue” is in fact quite observable. The instantaneous conductance of a photoconductive cell depends upon the device’s previous exposure to light and the duration of that exposure. The magnitude of the effect is

p. 54

dependent upon several operating conditions: a) the present light level, b) the difference between previous and present illumination levels, and c) the durations of previous and present exposure. Whether the conductivity is higher or lower than expected (the sense) depends on previous illumination (lower or higher, respectively). In other words, the material “remembers” previous illumination levels by exhibiting a present conductivity dependent upon the direction from which the conductivity point was approached. Of course, in time an equilibrium value is approached asymptotically. “Light History” effects are plotted for two types of Cadmium Selenide material in Appendix XIV [74]. To understand this graph, consider a specific material at an instantaneous operating point: Type 4, 0.1 foot candles. If the cell was previously stored in total darkness for a “sufficiently long” time, the device will exhibit a conductance 1.5 times greater than if it had been stored for a “sufficiently long” time under 30.0 foot candle illumination. “Sufficiently long” refers to elapsed times which are orders of magnitude beyond normal relaxation time. The photoconductor manufacturing industry refers to this as “infinite” time. This so called infinite time is usually measured in seconds and most often is less than one minute.

Type 4 Cadmium Selenide material exhibits low light history effects. Many Cadmium Sulfide compounds exhibit even lower levels of the light history effect. However,

p. 55

notice that the light history effect is less marked at high levels of illumination. Since the anticipated illumination levels for the microwave photoconductor would be moderate (1.0 foot candle) to high (100.0 foot candles), Cadmium Sulfide offers little improvement over Cadmium Selenide with regard to light history. The Type 4 Cadmium Selenide material is also known to exhibit a smaller relaxation time than Cadmium Sulfide compounds. Speed of response must be regarded more important than absolute light history.

4.1.3 Speed of Response

The response speeds of commercial photoconductors are normally specified in terms of a time constant. Thus, the quoted rise time is that time required for the device current to reach 63.2% of the final value after a specified illumination is initially applied from total darkness. Similarly, when the specified illumination is totally removed, the decay time is noted to be that time for the device current to reach 36.8% of the final dark current [75]. The Type 4 Cadmium Selenide material utilized in this research exhibits response times depicted in Chart 4.

Notice that the material responds faster at higher levels of illumination. This is typical of photoconductive compounds. For fast conductive transitions, it is possible to wave shape the envelope of the driving optical signal: For example, sudden high brilliancy followed by a lower

p. 56

quiescent illumination level. Other more exotic photoconductive compounds are capable of response times down to the nanosecond level. At least one team of investigators [97] has successfully demodulated microwave information from a laser beam using a photoconductive cell. For automotive radar applications, the response times for Cadmium Selenide should prove adequate. This statement is supported by three system considerations: a) algorithm processing time; b) receiver operating characteristics (ROC), transmitted power, and antenna beamwidth; and c) vehicle dynamics.

Chart 4 — Type 4 Cadmium Selenide Response Times

Illumination (foot-candles) Rise Time (milliseconds) Decay Time (milliseconds)
0.01 400.0 90.0
0.1 90.0 36.0
1.0 35.0 18.0
10.0 10.0 9.7
100.0 3.0 5.0

For the first consideration (algorithm processing time) it must be recognized that the digital computer has an upper limit (in time) for determining an output response. Information should not be supplied at a rate exceeding the processing speed. Present microprocessors have clock frequencies which range between 1.0 and 10.0 Megahertz. For

p. 57

elementary algorithms, such as the phase plane boundary technique, 250 clock cycles may be required. This corresponds to processing times between 0.25 and 0.025 milliseconds, respectively. If pattern recognition (target signature) is invoked, these times will increase by at least two orders of magnitude.

Receiver operating characteristics, transmitter output power, and antenna beamwidth are salient factors pertaining to a maximum permissible scan rate. Based upon confidence limits imposed on the ability to detect specified targets, it may be analytically demonstrated that the scan rate (inverse of search time) assumes a maximum limit. This formulation is put forth in Appendix XV. Actual numerical values are not used in this formulation as system performance requirements are still the subject of much research. However, given a target (radar cross section), receiver operating charcteristics (this includes the probability of detection versus the probability of a false alarm), transmitter power and modulation format (pulse duration), and antenna beamwidth (gain), minimum search time () may be determined for a maximum range to target. Calculations based upon reasonable system requirements (such as the Bendix research vehicles) indicate search times not lower than a few milliseconds.

Vehicle dynamics are elegantly simple to understand. For example, let us say that a vehicle is heading for an

p. 58

impending mishap at a closure rate of 160 kilometers/hour (100 MPH). If the target is acquired in 10 milliseconds the vehicle has only advanced 0.447 meters (17.6 inches).

It should now be clear that the Cadmium Selenide material is entirely satisfactory in terms of speed of response for automotive radar beam scanning when operated at moderate to high optical levels.

4.1.4 Spectral Response

Appendix XVI depicts the typical normalized optical response of Type 4 Cadmium Selenide material. It is noted that the peak spectral response occurs at a wavelength of approximately 690.0 nanometers (red in color). Gallium Aluminum Arsenide (GaAlAs) light emitting diodes (LEDs) exhibit optical outputs quite close to this wavelength band. The peak optical output for these emitters occurs at a wavelength of approximately 660.0 nanometers. Yet, between the photoconductor’s optical spectrum and the emitter’s optical spectrum, there exists significant overlap. See Appendix XVII. The selection of the Gallium Aluminum Arsenide emitter was therefore an obvious choice. Data Display Products of Inglewood, California, 90302, was very kind to supply high efficiency, high brightness experimental emitters. These devices are of the GaAlAs variety, but with integral prefocused lenses. The typical optical output for each diode is specified to be 0.500 candelas (0.490

p. 59

candles) for a forward current of 0.020 amperes. Variation of the LED luminous intensity with applied forward bias (transfer characteristic) is depicted in Appendix XVIII. When the experimental beam steerable antenna was constructed, the specified emitters were positioned within 0.3 inches of the photoconductive surface. Forward current control is provided between 0.25 milliamperes and 19.75 milliamperes on the demonstration unit’s diodes. The nominal midscale diode current was established at 9.75 milliamperes.

4.2 Device Configuration

Commercial photoconductive cells are normally fabricated in three layers: a) the substrate (Alumina), b) the photoconductive compound, and c) the ohmic contacts (Indium). The channel formed between the ohmic contacts in the plane of these contacts exposes the photoconductive compound to optical radiation. The channel may be fashioned in a straight line or as a meandering path. The latter configuration is achieved by interdigitating “fingers” of the ohmic contacts. It provides for long channel linear lengths and establishes a low device resistance. Low device resistance may be attained by long channels and/or narrow width channels. Upon examination of a commercial photoconductive cell its appearance is not unlike a lumped element (LE) microwave capacitor [2]. See Fig. 1 of

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Appendix XIX. This observation prompted the following goal: to fabricate a “universal” microwave photoconductive device. If such a universal device could be realized, its application would not be limited to the Apparent Geometry Modification antenna technique. In fact, beam steering could be accomplished with existing commercial planar antenna arrays by incorporating microwave photoconductors in the structure. Small (0.15 inch diameter) commercial photoconductive cells were considered as candidates for application at X band (8.0 to 12.0 Gigahertz). Several difficulties arise, however. First, even for the small chip (0.15 inch diameter) residual capacitance across the channel is quite high (~ 1.0 picofarad). At 10.0 Gigahertz this corresponds to a reactance of only around 16 ohms. This low value would clearly mask resistance variations of the photoconductor. Notwithstanding this difficulty, one might consider resonating the device with a shunt inductive element. However, at X-band it is necessary to evaluate the true equivalent circuit. For the capacitor itself, the interdigitated fingers exhibit inductive reactance. Capacitance is then distributed between adjacent fingers. See Fig. 2 of Appendix XIX. It is noted that this “capacitor” is in fact a network of distributed inductance and capacitance. For convenience, refer to this combination as capacitor “.” In Fig. 3 of Appendix XIX, an inductive shunt is added in parallel with . This inductive element

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passes directly through the substrate from the backside and makes electrical contact with both capacitor “plates.” Leads exiting the device exhibit inductance. The vertical components of the shunt through the substrate also exhibit inductance. The horizontal portion of the shunt exhibits inductive and capacitive characteristics. Capacitive coupling is achieved through the dielectric (substrate) to the interdigitated fingers of . Since the fingers of are interdigitated, crossed distributed capacitive coupling is achieved in addition to the progressive distributed capacitance. An accurate equivalent circuit model for this configuration is given in Fig. 4 of Appendix XIX. This arrangement exhibits a strong multimodal nature. Under swept frequency laboratory studies, numerous interlaced resonances and antiresonances were observed. Since the resonances were quite shallow (~ 2 dB in a 50 ohm transmission configuration), the three-dimensional device was abandoned from further study.

To avoid multiple modes in a microwave device, a symmetric, monolithic structure must be realized. Refer to Appendix XX. A cross section of this element reveals only three planar layers: the substrate (), the photoconductive compound (CdSe), and the top conducting sheet (Indium). The straight channel which communicates with two end holes provides for the lowest possible capacitance of all configurations. With the exception of

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this channel, conducting Indium extends over the entire top surface. Thus, around the outer edges of the holes are formed two identical flat inductive loops which shunt the coplanar capacitor. With this geometry, four electrical components may be identified: two end inductors (L), a low inductance coplanar capacitor (C), and a resistor (R) which represents the photoconductor itself. All four components appear in a parallel electrical configuration. This is depicted as network “A” in Appendix XXI. The two end inductors electrically combine to form an equivalent inductance value of L/2. This is shown as network “B” in Appendix XXI. This system is a parallel RLC circuit with a clearly defined resonant frequency. If the device is operated at this point of resonance, the magnitudes of capacitive and inductive reactances (X) are equal. However, since these reactances are imaginary with opposite signs ( negative, positive), the total impedance of the device reverts to pure resistance as provided by the photoconductor. See model “C” in Appendix XXI. In essence, the inductive reactance of the end inductive loops has effectively cancelled the capacitive reactance of the coplanar capacitor.

Electrical connections are made perpendicular to the channel and directly on to the conducting Indium. For the experimental devices which were fabricated, these connections consisted of silver epoxy bonds to flat copper

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conductors leading to center pins of type SMA connectors. This facilitated rapid testing and tuning. This technique would, of course, not be suitable for production units. Production units would incorporate integral microstrip connections with no bond.

The physical dimensions for the experimental units are as given in Appendix XX. A special test fixture was fashioned for testing device performance. The test fixture and its performance are described in a later section (4.4). The prediction of electrical parameters for the microwave photoconductive element are described in subsections 4.3.1 and 4.3.2.

4.2.1 Fabrication

The commercial Cadmium Selenide material was supplied by the manufacturer (Vactec, Inc.) deposited on an alumina () substrate. The task of supplying ohmic contacts was facilitated by vacuum deposition of conductive Indium metal. This was accomplished using a Varian VE-10 system at the Materials Research Laboratory of The Pennsylvania State University. Pieces of number 30 round copper wire (AWG, 0.01 inch diameter) were utilized for masking. Prior to chamber evacuation, these “masks” were laid from hole to hole on individual photoconductive blanks. Thus, Indium was deposited on all exposed chip surfaces. Of course, the chip underside remained Indium free. Also, Cadmium Selenide

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directly under the mask remained Indium free. The channel formed under the mask is clearly defined. This was confirmed by 400 power microscopic examination. The channel width was noted to be 0.006 inches. This reduced width was a consequence of overspraying a mask with a circular cross section. All edges of the fabricated chips were cleaned using 600 grit silicon carbide cloth. Indium within the holes was removed with number 73 drills and unwaxed silk dental floss. Electrical connections to the chips were made with flat copper ribbon. The bond is formed using a two-part silver epoxy system.2 Refer to Appendix XX for the physical configuration of the chip with connections.

4.3 Device Characterization

The fabricated devices behave as true lumped element RLC networks. This was confirmed by swept frequency analysis. For a device with dimensions as given in Appendix XX, a natural resonance around 16.85 Gigahertz is observed. For optical saturation of the photoconductor, a typical bandwidth (BW) of 555 Megahertz is noted. Experimental results are in good agreement with calculated expectations. The next two subsections demonstrate capacitance (4.3.1) and inductance (4.3.2) calculations.

p. 65

4.3.1 Intrinsic Capacitance Determination

Two coplanar electrical conductors give rise to electrical capacitance. The value of capacitance based upon physical dimensions of the conductors may be calculated by invoking a technique of linear conformal mapping [19]. This is necessary because electric flux lines extending from plate to plate are families of confocal ellipses. Similarly, equipotential surfaces are families of confocal hyperbolas.

Foci appear at inner plate edges. A Schwarz-Christoffel transformation [46, 80, 89] is suitable for capacitance calculation since this maps the coplanar configuration into a parallel planes configuration. The capacitance of one side of a coplanar capacitor is therefore given by:

where: - = capacitance in farads - = relative dielectric constant - = dielectric constant of free space farads/inch

and are complete elliptic integrals of the first kind:

and

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The argument m is the ratio of spacing of inner edges (gap width) to spacing of outer edges of the plates cross sections.

= length of plates (assumed to be identical)

The complete elliptic integrals have been computed with the aid of the IBM 370/3033 computer. Subroutines are offered by the International Mathematical and Statistical Library of Subprograms (IMSL) [40]. Subroutines for complete elliptic integrals of the first and second kind are named MMDELK and MMDELE, respectively.

On one side of the microwave photoconductive chip electric flux lines extend out into free space. Therefore, for this side the relative dielectric constant is taken as unity. On the reverse side, however, exists the alumina substrate. The relative dielectric constant and the loss tangent of the subject material are constant over the frequencies of interest. At X-band frequencies, in-house measurements revealed a relative dielectric constant of 8.61 ± 0.02. The loss tangent was noted to be on the order of . Both of these values were confirmed independently by the N.J. Damaskos Company of Concordville, PA, 19331.

A direct capacitance calculation using the complete elliptic integrals should not be attempted for the substrate

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side of the coplanar capacitor. This statement is a consequence of the substrate finite thickness. Thus, total electric field confinement within the substrate does not exist for the full width of the device. Accurate calculations are possible, however, with the aid of reasonable approximations and a suitable model. Refer to Appendix XX. First, the length of the channel will be taken from inner hole edge to inner hole edge (0.195 in. − 0.026 in. = .169 in.). Clearly, there must be additional capacitance across the holes. This contribution is negligible, however, because the diameter of each hole is significantly greater than the photoconductive channel width. Second, the total width of the coplanar capacitor does not remain constant. Notice that the length of the photoconductive channel extends past the flats on either side of the chip. The developed analysis will ignore this fact. This is appropriate since the device width is much greater than the photoconductive channel width. Thus, the altered ratio of elliptic integrals at the device edges will subtract little from overall capacitance calculations.

The geometric model put forth for capacitance calculations is depicted in Appendix XXII. Capacitance accounts for free space electric flux on one side of the device. For the opposite side, it is necessary to determine that width which represents boundary limits for total electric field confinement within the substrate. It is

p. 68

reasonable to address geometry alone. For an ellipse:

where: - = focus to focus distance - = semimajor axis length - = semiminor axis length

Taking f = 0.006 in. and n = 0.04 in., the semimajor axis is calculated to be 0.04011 in. Thus, total electric field confinement within the substrate extends over a width equivalent to 0.08022 inches. This contribution to total device capacitance is referred to as in the model. Electric flux lines which exist beyond the total field confinement region and inside the substrate are approximately parallel geometrically. Therefore, two capacitors () are depicted in parallel plate configurations. From considerations based on electric networks, it is seen that both of these capacitors () are in electrical series and this combination is in electrical series with capacitor . The capacitor , of course, is a consequence of free space electric flux linking both of the capacitors. Total device capacitance is therefore based on three contributions: , , and the (, , ) series combination.

Calculation of total device capacitance begins with determining from the complete elliptic integrals. The capacitance is determined in the following fashion:

p. 69

is calculated assuming the absence of the substrate. Each capacitance is found by the usual procedure which applies to the parallel plate configuration. Once again, however, the relative dielectric constant of the substrate is omitted. It may now be seen that:

where primes (’) indicate that the relative dielectric constant of the substrate is omitted. Rearranging terms, is found:

The capacitance is now determined:

These last two equations facilitate the calculation of capacitance contribution from the (, , ) combination to the total device capacitance. This contribution is defined as . Thus:

The capacitance is easily determined:

The total device capacitance is simply the sum of , , and :

p. 70

Complete calculations for total device capacitance are given in Appendix XXIII. Thus, the intrinsic capacitance of the device depicted in Appendix XX is determined to be 0.3231 picofarads.

4.3.2 Inductance Determination

Caulton [12] has quoted Dukes [20] for a suitable formula used in determining the inductance of flat single turn conducting loops:

where: - is in nanohenries - = outer circumference in mils - = width of conductor in mils - = conductor thickness in mils (1 mil = 0.001 inch)

note: - = permeability of free space nanohenries/mil - = outer radius of inductor in mils

The above formula assumes . It also predicts an inductance lower than the inductance for an equivalent length of straight flat ribbon:

p. 71

where = ribbon length

This formula has been given by Terman [96]. Once again, L is in nanohenries and all dimensions are in mils. The fact that the flat straight ribbon exhibits higher inductance than an equivalent length of ribbon in a flat single loop configuration is a consequence of the mutual inductance consideration for the loop [12, 58, 87]:

where: - = self-inductance - = coefficient of coupling - = mutual inductance

The end inductive loops of the microwave photoconductive device consist of an involved geometry. In order to use the inductance formula for a single turn conducting loop a concern arises: what values should be used for “” (the circumference) and “” (the conductor width)? This difficulty is resolved by observing that, within reasonable limits of accuracy, consistent results may be obtained over widely varying values of “”:

First, assume “” to be the smallest distance between the hole edge (point “”) and the device edge:

or

This implies a fictitious loop circumference of:

p. 72

or

These values are then entered into the inductance formula for a single turn conducting loop with the assumption that the thickness “” is negligible (t = 0). The following calculation results:

or

Second, if the hole perimeter is traversed from the point “” in either direction, “” is noted to increase with an attendant increase in circumference (). A sensitivity analysis is therefore performed. It is noted that if “” is selected to be twice the initially selected value, calculated inductance rises by less than 0.5 percent:

and

so,

or

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The width “” may be increased even further with little change in calculated inductance. See Appendix XXXII. Further, to verify that the flat single turn loop formula is appropriate in this application, an alternate scheme of inductance calculation was devised:

Consider a straight flat conducting ribbon of length equivalent to the hole circumference:

or

As before, consider “” at the narrowest point:

Using the formula which predicts inductance for a straight flat conducting ribbon, the self inductance of an end loop is calculated. Once again the thickness “” is taken as zero:

or

It is now necessary to account for mutual inductance of the loop. Ramo, Whinnery and Van Duzer [80] offer the method of selected mutual inductance for such a calculation:

p. 74

where: - = 0.021 inches (as before) - = (0.021 + 0.013) inches = 0.034 inches (the loop diameter)

and are complete elliptic integrals of the first and second kind, respectively. See 4.3.1 for the definition of . is defined as follows:

As in subsection 4.3.1, the integrals and are computed via IMSL subroutines MMDELK and MMDELE on the IBM 370/3033 computer.

Thus, for m = 0.8946:

or

It is now possible to calculate the total loop inductance (L):

or

or

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This value of inductance (0.5523 nanohenries) is extremely close to the value predicted by the Dukes formula (0.6074 nanohenries). In fact, the two values disagree by a little less than ten percent. Each of these calculations indicates that inductance estimates which are reasonably close to the exact value are possible. It is the lack of axial symmetry in the conduction plane, of course, which hampers the development of an exact solution method. Many researchers [12, 96] have experienced similar calculation difficulties for configurations with even higher symmetry. Many formulas for predicting inductance have been empirically formulated and are usually accurate over specified frequency and dimensional limits. In most situations, distributed capacitance accompanies the inductance. When one attempts to account for fringing and skin effects, the task of developing an exact analytic expression for predicting either capacitance or inductance is anything but trivial.

4.3.3 Tuning to Desired Frequency of Resonance

The fabricated microwave photoconductive devices exhibit a natural single frequency of resonance which may be predicted as follows:

The values of capacitance (C) and inductance (L) are those values predicted as in previous subsections (4.3.1 and 4.3.2). The effective inductance (L/2) entered into the

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well known resonance formula is a consequence of the two inductive end loops shunting the coplanar capacitor. For the fabricated chips (dimensions given in Appendix XX), the point of resonance may be calculated:

Actual measurements indicated a slightly higher resonant frequency (~ 16.85 Gigahertz). Two separate batches yielded chips with resonant frequencies matching within the limits of repeatable accuracy. All measurements utilized mechanically tuned frequency meters (Hewlett Packard models X530A and P532A) [22].

Clearly, the device resonant frequency may be specified a priori. The geometric dimensions would then be selected to produce this point of resonance. This would be the preferred method suitable for commercial manufacturing. This luxury was not afforded the experimental investigation being described. Since it was desired to produce demonstration devices which would resonate in the X-band (~ 10.5 Gigahertz), a method of tuning the devices after Indium deposition was sought. If a flat conducting strip is placed across the backside of the microwave photoconductive substrate it is possible to alter both capacitance and inductance. By changing the position of this conducting

p. 77

strip the point of resonance may be varied continuously. The fact that device capacitance is altered is easily understood: Electric flux lines which would otherwise extend out into free space in an approximately elliptical fashion are now confined under the conducting strip. This strip along with conducting Indium on the other side of the microwave chip form two series connected parallel plate capacitors. The dielectric separating the parallel plates, of course, is the device substrate. The net effect of the conducting strip’s presence is to increase device capacitance. The resonant frequency of the device is therefore lowered from its original previous value. It may be demonstrated, however, that if the entire backside of the device is supplied with a conducting plane the increased capacitance is insufficient to lower the point of resonance down to the desired 10.5 Gigahertz frequency. Yet, a brass strip (0.30 inches x 0.060 inches x 0.020 inches) laid flat on the device backside could be positioned such that any frequency from below 9.0 Gigahertz up to the natural untuned frequency (~ 16.0 Gigahertz) could be achieved. The lower frequencies occurred when the brass strip was brought in proximity or partially over the device end holes. Since device capacitance may only be increased to a limit, the lower resonant frequencies are a consequence of increased device inductance. It is clear that the flat tuning strip exhibits local circulating currents induced by the magnetic

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fields of the inductive end loops of the device. These currents produce an opposing magnetic field which is capable of bucking the mutual inductance contribution of the device end loops. This confirms two previously stated facts: a) The flat single turn conducting loops exhibit lower total inductance than equivalent lengths of flat conducting ribbon of equivalent width, and therefore: b) The total inductance calculation for each conducting loop must include the mutual inductance term which appears as a negative entry ().

Two microwave photoconductive chips are utilized in a demonstration beam steerable antenna. Since it was desired to operate this antenna at a frequency of approximately 10.5 Gigahertz, it became necessary to tune both chips to the same resonant frequency. Further, once the desired resonance points were established, a method for maintaining the devices at this frequency was necessary. This was achieved by bonding brass strips (tuners) to the backsides of the chips. See Appendix XXIV. These tuners were fashioned from 0.020 inch thick sheet stock. The finished tuners measured 0.30 inches (length) x 0.060 inches (width) x 0.020 inches (thickness). A two-part epoxy cement facilitated bonding.3 Other kinds of glue proved unusable for several reasons. Cyanoacrylate alters apparent dielectric

p. 79

characteristics and affords no additional adjustment time after application. Other glues suitable for plastic bonding change dielectric properties as they harden. They also exhibit “memory.” That is, if the tuner was repositioned during the glue cure cycle it would be returned to its original position by the glue. The two part epoxy system achieved the desired metal to ceramic bond and afforded tuning adjustments throughout the cure cycle. Each device was continuously monitored for proper resonance over five hour periods. Small corrective frequency shifts during the cure cycles produced two devices matched within 25.0 Megahertz at bogey resonances of 10.525 Gigahertz. This corresponds to tuning accuracies better than 0.25%. The optically saturated electrical bandwidth for these devices was measured and found to be ±350.0 Megahertz. This corresponds to a “Q” of 15.0.

4.4 Test Fixture Characteristics

Successful testing of the microwave photoconductive chips requires a standard test fixture. This is necessary to secure reproducible results at the frequencies of interest. In early experiments, type N bulkhead connectors were used in a back to back configuration. These connectors have quite large dimensions and therefore afford little connector to connector isolation. Shielding hoods were used to achieve isolation at the expense of introducing

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undesirable modes to the fixture. A superior fixture was devised utilizing the smaller SMA bulkhead connectors.

The test fixture used for all measurements was ultimately incorporated into the demonstration antenna system. This fixture accommodates two microwave photoconductive chips simultaneously. The test fixture is constructed from two aluminum blocks which are each 0.186 inches thick. Each block surface (1.6875 in. x 0.575 in.) mounts two SMA bulkhead connectors (for a total of four connectors) with 4-40 hardware. The blocks are maintained apart by 0.25 inches using 0.19 inch diameter aluminum spacers over the same machine screws which mount the bulkhead connectors. Thus, a 0.25 inch channel is formed between the aluminum blocks. This dimension accepts the microwave photoconductive chips with 0.0135 inch clearance on each side. Two chips reside isolated in the fixture on centers appearing 1.125 inches apart.

No attempt was made to fabricate a test fixture which would maintain a constant impedance. Dispensing with a constant impedance requirement was necessary to achieve flexibility in chip tuning (see subsection 4.3.3). More important considerations deal with the maintenance of uniform amplitude transmittance over the frequencies of interest (conducting chip present) and high electrical isolation (conducting chip absent). These two parameters were tested for each side of the test fixture (NO DOT END

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and DOT END) over the frequency range of 8.0 Gigahertz through 12.4 Gigahertz. See Appendix XXV. Two blank chips were fashioned with Indium covering one side of the substrate entirely. These chips bonded into the test fixture permitted measurement of amplitude transmission characteristics. The resistances caused by the silver epoxy bonds were noted to be 0.4 ohms and 1.2 ohms (NO DOT END and DOT END, respectively). Up to 11.0 Gigahertz, less than 2.0 decibel variation is noted in transmission for both sides of the fixture. Out to 12.4 Gigahertz maximum amplitude variation is approximately 3.0 decibels (total) for either side. Isolation (chip removed) for either fixture position is better than 50 decibels. For all measurements, the amplitude/frequency characteristic of the crystal detector was taken into account.

For the frequencies of interest, the chip and test fixture must be considered as a unitary system. Amplitude transmission characteristics may be adversely influenced by geometric alteration of the center line conductor (the chip) or the test fixture. For the sake of completeness, this phenomenon is also demonstrated in Appendix XXV. By replacing the blank chips with cylindrical conductors (0.0159 inch diameter), it is noted that the transmission characteristics for either position of the test fixture are greatly affected. Wide amplitude excursions (5.5 decibels) are noted for small frequency shifts (10.7 to 11.0

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Gigahertz). The effect is even more pronounced (~ 8.0 decibels) at higher frequencies (11.0 to 12.3 Gigahertz).

The foregoing analysis is necessary for proper interpretation of tests performed on the microwave photoconductive chips. Without measurements of the test fixture alone, ambiguity would result. Thus, based upon the predictable performance of the test fixture, any observed resonance may only be attributed to the chip under test.

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CHAPTER 5

RADIATING STRUCTURE DEMONSTRATION

5.1 Bihorn Array

Development of the microwave photoconductive elements proved to be entirely successful. It is therefore logical to demonstrate the applicability of the devices in their initially intended function: electromagnetic beam steering. In order to accomplish such a demonstration, a radio frequency (RF) radiating structure must be established. Apparent Geometry Modification (AGM) of a single radiating element would be most impressive. AGM would, however, require the fabrication of an integrated electromagnetic radiator/photoconductor. Local facilities for such fabrication are unavailable. Yet, on-hand fabricated microwave photoconductive chips could be incorporated into an easily constructed array. This latter suggestion demonstrates wide versatility. Existing antenna array technology could be expanded to accept microwave photoconductive elements. Selection of a suitable radiating structure was based on two criteria: simplicity and reasonably high gain (directivity). Simplicity facilitates fabrication. On the other hand, high gain permits ease of observation with regard to beam steering. That is, the

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primary lobe of a low directivity antenna is quite bulbous. Because of the low amplitude to angle gradient of such a radiator, main beam steering may be difficult to observe. This is especially true at the angle of highest gain (head on). Thus, high gain structures are desirable for demonstration purposes because of dramatic steering effects. No attempt was made to secure the gain requirements of automotive radar. This would require unnecessary expenditures in time and cost. A modest two element phased array ultimately was selected to be the preferred demonstration candidate. Referring back to section 3.2, it is noted that the described wire fed horn (2.0 wavelengths long leading edge) achieves a very respectable forward gain of 13.33 dB above an isotropic radiator. However, a beam steerable phased array requires individual radiators to be placed at odd multiples of half wavelengths. Therefore, if the leading edge of such a horn could be shortened slightly to 1.4 wavelengths (while maintaining the same aspect ratio), two identical radiators could be positioned 1.5 wavelengths apart, side by side in the same plane, establishing a Bihorn structure.

To assist comprehension of individual array elements, refer back to Appendix IX. Recall that the depicted horn is first developed in the XY plane. The leading edge is 2.0 wavelengths long. The distance from the leading edge to the feed point is 1.5 wavelengths. If the leading edge is

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shortened to 1.4 wavelengths, the distance from the leading edge to the feed point becomes 1.05 wavelengths. Thus, the original aspect ratio is maintained. This shortened horn (as before in section 3.3) is rotated about the Y axis by 41.81 degrees:

A perfect imaginary pyramid is thus established with the image reflected in the XY ground plane. In fact, the open sides which exist between the edges of the radiator and its image are of the same dimensions as the radiator or its image. That is, the leading edge of the radiator taken with the leading edge of the image form a square mouth. The geometric similarity between these radiators and the Great Egyptian Pyramid of Gizeh prompted my colleagues to refer to the large horn (2.0 wavelengths leading edge) as the Pharaoh. The smaller horn (1.4 wavelengths leading edge) naturally was nicknamed Mini Pharaoh.

The radiation characteristics of the Mini Pharaoh were determined with the aid of the antenna modelling program (AMP). Refer to Appendix XXVI. The main lobe exhibits a forward gain of 12.64 dB above an isotropic radiator. Feed point impedance was noted to be 84.26 + j73.99 ohms.

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5.1.1 Bihorn Characteristics

Consider a single isotropic radiator fed with unit power . The radiation pattern which results in any plane is a circle. This circle may be regarded as a reference with nomenclature 0.0 dB. If two isotropic radiators are spaced apart by 1.5 wavelengths and each fed with unit power , the corresponding array factor (AF) which predicts the far field intensity along any plane intersecting the midpoint of a fictitious line joining the sources is easily calculated [92]. Consider a plane crossing this line at its midpoint. An angle () is defined between the line and the plane. Let be the electrical (excitation) phase displacement between radiators. Then:

or

but

so

If is taken to be zero (excitations in phase), the radiation pattern which results is plotted in Appendix XXVII. For the demonstration antenna system, the isotropic

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radiators are replaced by Mini Pharaoh horns. If mutual coupling between the two radiators did not exist the resulting radiation pattern could be synthesized from the technique of pattern multiplication [44]. That is, the radiation pattern of the individual radiators would be multiplied by the array pattern. Since interaction between the radiators is known to exist, AMP was again called upon to predict the Bihorn far field radiation pattern with respect to azimuthal angle (horizontal plane). Results are depicted in Appendix XXVIII. Two AMP simulations for this system with different excitations permitted determination of open circuit impedance parameters. Treating the feed points as a two port network:

The equation for the array factor (AF) suggests the means for accomplishing beam steering. For this configuration, lobe maxima may be predicted as follows:

or

Thus, for in phase excitation () the main beam is at a right angle with respect to the fictitious line joining

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point source radiators. Because the array is developed in quadrants II and III of the XY plane, the main beam peak resides at 180.0 degrees for in-phase excitations.

5.2 Demonstration Equipment

The Bihorn radiating structure (copper) is fashioned on glass epoxy substrate of 0.060 inch thickness. The nominal relative dielectric constant of this material is 2.5. The Mini Pharaoh radiators are fed with a common phasing line. The phasing line is 0.086 inch wide microstrip. The effective surge impedance and effective relative dielectric constant for this line are obtained from tabulations [36]:

Refer to Appendix XXIX. The phasing line is provided excitation at two points spaced 0.3 inches apart. The microstrip feed lines are 0.174 inches wide and achieve surge impedance values of 50.0 ohms. All other RF system connections are accomplished with rigid 50.0 ohm coaxial lines. It may be seen that an X-band Gunn source4 feeds RF energy to a Wilkinson type power divider.5 The

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commercial Gunn source combines varactor tuning facilities along with an integrated circuit voltage regulator (MC 1569) and series pass transistor (2N3997). In order to permit the source to accept square wave (1000.0 Hertz) pulse modulation, three modifications were performed: The integrated circuit regulator speed was increased by removal of a 0.1 microfarad noise suppression capacitor, the series pass transistor response was improved by removal of a 15.0 microfarad emitter capacitor, and additional heat sinking (aluminum) was provided for the GaAs Gunn element module. The subject microwave source is capable of supplying continuous (CW) output power of approximately 60.0 milliwatts at a frequency of 10.5 Gigahertz.

Two in-phase microwave signals are provided from the power divider output ports. These signals are applied to small ferrite isolators6 (circulators with matched 50.0 ohm terminations at port 3). These isolators prevent reverse power feed for high voltage standing wave ratios (VSWR). Thus, as feed forward power is varied by the microwave photoconductor, interaction between power divider output ports is avoided.

The microwave photoconductive elements reside between the outputs of the isolators and the 50.0 ohm microstrip

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feed points which connect to the phasing line of the Bihorn array.

If the two in-phase excitations at the phasing line are of equal amplitude, a single virtual feed exists at the phasing line midpoint. Thus, the main beam is radiated straight ahead (180.0 degrees) as depicted in Appendix XXVIII. However, if the photoconductive elements are illuminated with unequal levels of light, the devices provide unequal amounts of attenuation. Thus, the two excitation signals appearing at the phasing line of the Bihorn array remain in-phase but are of unequal amplitude. By phasor addition it is seen that the single virtual feed point has been shifted from the midpoint of the phasing line. This shift establishes an electrical phase displacement of signals which arrive at individual radiators. Thus, beam steering is achieved in accordance with the equation specified for the array factor (AF).

Appendix XXX describes the electrical circuitry necessary to augment the Bihorn radiating structure as a complete microwave transmitter. The schematics indicate three regulated power supplies, current steering control for the light emitting diodes which excite the microwave photoconductors, and the square wave pulse modulator which supplies the Gunn microwave source. An avalanche diode (1N2999A) establishes regulated voltage for the tuning varactor within the Gunn microwave source. Frequency tuning

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is accomplished via a ten turn 10.0 kilohm linear taper potentiometer (0.0 − 48.0 volts). Two integrated circuit voltage regulators (LM317) provide 15.0 volts D.C. power to the modulator and the light emitting diode (LED) circuitry. LED currents are steered via series/shunt resistance arms. Variation is affected by a 10 turn 1.0 kilohm linear taper potentiometer. When this control is physically centered, equal currents are established through the diodes. If the potentiometer setting is changed, one diode receives higher current while the other diode current is diminished. Full range current control for each diode spans 0.25 to 19.75 milliamperes as monitored by two individual analog meters. Provision is made for turning off the light emitting diodes completely by a DPDT switch. In the LED off position, the meters double as voltage monitors for the regulated power supplies (self diagnostic).

The modulator section of the microwave transmitter uses a CMOS integrated circuit timer (ICM7555) connected to achieve astable operation. Frequency of modulation is adjustable via a ten turn 100.0 kilohm linear taper rheostat. A square wave with a 50.0 percent duty cycle (approximately) may be achieved over the frequency range of 635 to 1555 Hertz. This frequency range was established so that the modulation frequency could be adjusted to the receiver’s tuned passband. (The receiver consists of a horn antenna with 17.0 dBi gain, a crystal rectifier, and a tuned

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AC coupled vacuum tube voltmeter (VTVM). The rectifier is a detector exhibiting square law transfer characteristics. The VTVM (Hewlett Packard, Model 415B VSWR indicator) is tuned to a nominal center frequency of 1.0 kilohertz.) The modulator is completed by a pulse amplifier consisting of complementary symmetry output transistors (2N6049 and 2N3054A) fed by three small signal drive/predrive transistors (all 2N2222).

5.3 System Performance

In order to predict the beam steering capability of the demonstration antenna, measurements were first performed on the microwave photoconductors in a matched 50.0 ohm system. The relative range of attenuation secured for total darkness to optical saturation (> 150.0 foot candles) for either of the two devices was noted to be approximately 10.0 decibels. Maximum LED optical output is considerably below saturation levels for the photoconductors. The reference RF signal level (0.0 dB) was established at an LED current of 9.75 milliamperes. If the LED current is reduced to 0.25 milliamperes, the relative RF signal falls to −3.5 decibels. If the LED current is raised to 19.75 milliamperes, the relative RF signal rises to +1.0 decibel. The observed asymmetry is indicative of the extreme non-linear characteristics of the LED and photoconductor. Accompanying relative RF voltage levels for the three test conditions are

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calculated:

5.3.1 Predicted Performance

Recall that the excitation feed points on the phasing line which connects individual radiating elements are apart by 0.3 inches. In terms of electrical length (), this corresponds to:

where: - = velocity factor - = wavelength

At a frequency of 10.525 Gigahertz, the corresponding free space wavelength is 1.1222 inches. The velocity factor is obtained from the effective relative dielectric constant:

or

Thus,

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or

Therefore, each feed point is observed to be away from the midpoint of the phasing line:

This information along with applicable RF voltage levels permit phasor estimations. Phasor addition assuming matched conditions (constant impedance) are carried forth in Appendix XXXI. The corresponding electrical phase displacements may then be supplied to the array factor formula to estimate the maximum steering angle achieved by the array:

5.3.2 Observed Performance

A testing platform enabled experimental observation of the demonstration radiating system. The platform consists of a small laboratory table with a radial (U-channel) aluminum arm. One degree increments are marked on the table surface. At the end of the radial arm is mounted an

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adjustable stand off tower which mounts a vertically polarized (E-field) horn antenna with 17.0 dBi gain. The WR90 flange of this horn mates with a waveguide end short cavity which contains a crystal rectifier. This rectifier provides “square law” detection characteristics. That is, the detector output voltage is proportional to the square of the RF input voltage. Absolute calibration is not required. The audio output of the detector is impressed at the input of a tuned single frequency vacuum tube voltmeter (Hewlett Packard Model 415B). This indicator is capable of 70.0 decibels dynamic range at the passband frequency (1.0 kilohertz).

The pivot point for the testing platform’s radial arm is positioned directly beneath the leading edge of the Bihorn transmitting antenna. The receiving horn is positioned at the same height as the transmitting antenna. The distance between the leading edge of the transmitting antenna and the leading edge of the receiving antenna is established at 36.0 inches. Thus at the operating frequency (10.525 Gigahertz) all measurements represent far field characteristics.

To insure proper frequency of operation, LED turn off provisions are included in control electronics. Thus, with the photoconductors darkened it is possible to adjust varactor bias within the Gunn microwave source. At resonance, a pronounced “dip” is noted in system radiation.

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with this accomplished, control may be returned to the light emitting diodes. Modulation frequency is adjusted to correspond with the VTVM passband by tuning to maximum meter deflection. LED currents are varied and beam maxima are sought by repositioning the radial arm. Prior to data recording, boresight alignment was accomplished by carefully positioning the radiating structure on the measurement platform.

With equal LED currents, forward antenna emission characteristics were observed to be in accordance with the expected plot (see Appendix XXVIII). As LED currents were varied, the main beam was noted to be repositioned in space. The steering characteristics obtained for the experimental arrangement are documented in Chart 5.

Chart 5 — Observed Beam Steering

LED 1 Current (milliamperes) LED 2 Current (milliamperes) Steering Angle (degrees off boresight)
19.75 0.25 +3.0
17.00 2.75 +2.0
14.50 5.00 +1.5
9.75 9.75 0.0
5.00 14.50 −1.5
2.75 17.00 −3.0
0.25 19.75 −4.5
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Steering of course occurs in a continuous manner. Measurements at angles much finer than single or half degree increments are difficult, however, because of the bulbous nature of the steered lobe. Also, linear steering characteristics should not be expected. Both the LED and photoconductor exhibit strong nonlinear transfer characteristics (refer back to Appendices XIII and XVIII). A slight asymmetric skew is experienced between steer left and steer right control sensitivities. This is a consequence of imbalances occurring between feed lines at the transmitter, mismatches between photoconductors, and differences in individual LED characteristics. Such imperfections are expected in experimental models intended to demonstrate feasibility alone. Industrial manufacturing tolerances would be much tighter, resulting in significantly higher symmetry.

It should be observed that the total angular beam displacement secured (3.0 + 4.5 = 7.5 degrees) is significantly lower than the theoretical prediction (7.08 + 7.08 = 14.16 degrees). This discrepancy is explained by recalling assumptions which led to the predicted steer angle. First, relative RF voltage output levels from the photoconductors were obtained in a matched (input and output) 50.0 ohm system. The antenna phasing line and associated feed lines present anything but a constant 50.0 ohm impedance to the photoconductive elements. Second,

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amplitude to phase conversion calculations (see Appendix XXXI) were based on constant impedance conditions. Linear addition of voltage phasors presupposes that constant impedance is maintained. The photoconductive elements vary resistance in accordance with applied illumination. Thus, the direct connection of the photoconductive elements to the antenna feed lines prohibits maintenance of constant impedance on the feed lines or phasing line. Estimations and observations can only be in agreement for the constant impedance condition. Otherwise, the effect of changing voltage standing wave ratios (VSWR) would have to be accounted for in all calculations. Such a rigorous analysis would be tedious. The intent of the predictions provided serves as first order estimates only.

Appendix XXXIII provides photographic documentation of the microwave photoconductive element, the antenna with associated RF components, the microwave transmitter control unit, and the receiving horn antenna used during system testing.

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CHAPTER 6

CONCLUSION

6.1 Summary Remarks

At the onset of the presented research, the utility of an effective consumer oriented collision avoidance automotive radar system appeared promising but for the high false alarm rate. This has been adequately documented via a complete television production. The subject radar system incorporated no provision for steering the emitted electromagnetic beam with respect to the vehicle. The beam steering provision yields the highest gain in system performance enhancement. Yet, this area has heretofore received little to no attention. This is understandable since cost effectiveness must be considered for successful implementation. Thus, the high challenge level provided impetus for study area selection. The developed method of antenna beam steering has the potential for making the previously most expensive system component the least expensive. The breakthrough was made possible by merging existing and established technologies. Apparent Geometry Modification (AGM) and microwave photoconductors are, however, of limited application. Yet, within these applications it is indeed difficult to imagine any other

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methods competing successfully on all salient considerations. Low power short range radar systems represent the most appropriate class of application for the microwave photoconductor. This research area proved most rewarding. Exhaustive literature searches7 proved that no previous investigator has considered using photoconductors as parts of an antenna system. Even more surprising is the fact that no other previous investigator has considered development of a universal microwave photoconductive element which could be applied as a light controlled microwave attenuator. Extensive literature searches by Dialog Information Services, Inc. revealed nothing comparable or even similar to the presented technological contribution. The microwave photoconductor should prove even more versatile in a host of related high technology applications. Signal processing at ever increasing frequencies should inspire continued research in this exciting area. Secondary features of photoconductive compounds may provide solutions to otherwise overwhelming requirements. For example, in terms of nuclear hardness, the junctionless photoconductor is comparable to a carbon resistor. At least one team of researchers [91] has studied the effects of 3-10 MeV accelerated electrons on CdS and CdSe. Radiation doses of

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rads. have been reported to enhance material crystal structure with attendant improvements in electrical properties. Thus, based upon inherent nuclear hardness and insensitivity to electromagnetic pulse (EMP) environments, the microwave photoconductor could find application in a battlefield tactical radar system.

6.2 Recommendations for Further Research

This research effort has been by nature interdisciplinary. Consequently, limited time was expended on individual constituent areas. The decision not to dwell on any supporting area was made during early research phases. This decision was necessary because the ultimate project goal was to culminate in the construction of a realizable product. The developed beam steerable antenna obviously is not suitable for immediate automotive radar application. It is a feasibility demonstration model only. A practical automotive radar system would address the development of a totally integrated RF subsection [35]. Thus, the antenna, the photoconductors, the RF source, the detector, and controlling electronics would exist on a single substrate. Reliability and cost effectiveness dictate this approach. The presented research relied on commercially available subassemblies and devices which could be fabricated with resources on hand. Although good reliability was realized, cost effectiveness was given no

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consideration. Areas meriting further research are not difficult to identify.

Apparent Geometry Modification (AGM) is an exciting area which needs much attention. So little has been accomplished in this area. A single radiator (not an array) which incorporates an electronically adjustable radiation pattern will offer many new application possibilities. Analysis and synthesis methods will have to complement material developments in order for this technique to realize full potential. AGM should be of interest to antenna designers from academic and practical considerations alike.

Microwave photoconductors are applicable to presently existing antenna array technology. Optimization of an array suitable for automotive radar applications would provide an immediate cost effective beam steerable antenna. For minimal commercial effort a high performance radiating system could be had. Dialogue between antenna fabricators and photoconductor manufacturers would have to be established, however.

Cadmium Selenide (CdSe) proved to provide good performance at X-band microwave frequencies. More research should be conducted on this material at even higher frequencies (up to and beyond 100 Gigahertz). Improved fabrication methods for this and other photoconductive compounds should be explored specifically for microwave applications. The geometry used for the presented research

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is very close to optimum because of low device capacitance. However, a substrate with a lower relative dielectric constant could be used to good advantage at millimeter wavelengths. For example, quartz [11] with a relative dielectric constant of 4.0 would be a better substrate candidate at higher frequencies. Consider the fabricated devices presented in this research. By scaling down the physical dimensions, resonant frequencies corresponding to millimeter wavelengths may be achieved. Even higher frequencies may be realized with a quartz substrate.

The inductive end loops utilized in the fabricated devices provided a high degree of tuning flexibility. The loop configuration also establishes repeatable inductance values, even for rudimentary fabrication methods. However, straight line channel shunting inductors can provide lower values of total device inductance. Thus, higher resonant frequencies are possible with straight line inductors which are physically short (the channel width). The success of a device utilizing such inductors resides in adherence to narrow margins of manufacturing tolerances. Producing devices with straight line inductors may lead to wide variations in device resonant frequencies. In fact, the resonant frequency of the device could be used as an indicator of manufacturing tolerances. This obviously requires further study.

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Finally, many advanced solid state device fabrication techniques are available. However, nearly all of these techniques are dedicated to transistor and integrated circuit production. The successful commercial manufacture of microwave photoconductors must consider the full gamut of existing production methods. Obviously, an assessment of volume requirements is dictated. Widespread application of collision avoidance automotive radar could warrant dedicated production facilities.

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  3. Pramanick, Protap and Gupta, Chimnoy Das. “Thin-Film Measurement Dispels Dielectric Doubt.” Microwaves 21 (January, 1982): 76-81, 84.
  4. Raff, Samuel J. Microwave System Engineering Principles. Oxford: Pergamon Press, Inc., 1977.
  5. Ramo, Simon, Whinnery, John R., and Van Duzer, Theodore. Fields and Waves in Communication Electronics. New York: John Wiley and Sons, Inc., 1965.
  6. Reindel, John. “Printed WG Circuits Trim Component Costs.” Microwaves 19 (October, 1980): 60-63.
  7. Rivard, Jerome G. “Microcomputers hit the road.” IEEE Spectrum 17 (November, 1980): 44-47.
  8. Satellite Communication Radio Astronomy and Radar. Design and Construction of Large Steerable Aerials. Conference Publication no. 21. Middletown, Pennsylvania: Wert Bookbinding, Inc., 1969.
  9. Schiller, T. R. and Heath, W. S. “An Electronically Scanned Array at Millimeter Wavelengths Employing Ferrite Apertures.” IEEE Transactions on Antennas and Propogation AP-16 (March, 1968): 180-187.
  10. Schwartz, Mischa. Information Transmission, Modulation, and Noise. Brooklyn Polytechnic Institute Series. New York: McGraw-Hill Book Company, Inc., 1959.
  11. Signetics Digital Linear MOS. n.p.: Signetics Corporation, 1972.
  12. Slurzberg, Morris and Osterheld, William. Essentials of Electricity for Radio and Television. Second Edition. New York: McGraw-Hill Book Company, 1950.
p. 112
  1. Smith, R. W. “Some Aspects of the Photoconductivity of Cadmium Sulfide.” RCA Review 12 (September, 1951): 350.
  2. Smythe, William R. Static and Dynamic Electricity. Third Edition. New York: McGraw-Hill Book Company, 1968.
  3. Society of Automotive Engineers. “Speedometer Test Procedures - SAE J1059-SAE Recommended Practice.” SAE Handbook 1976 Part 1 Materials Parts and Components. Warrendale, Pennsylvania: Society of Automotive Engineers, Inc, 1976.
  4. Spinulescu, I., Ruxandra, V., and Baltateanu, N. “Effect of ionizing radiations on the electrophysical properties of the thin layers of cadmium senide and cadmium sulfide.” An. Stiint.Univ. “Al. I. Cuza” Iasi. Sect. 16 vol. 27, pp. 13-18, Univ. Bucarest, Bucharest, Romania, 1981.
  5. Stutzman, Warren L. and Theil, Gary A. Antenna Theory and Design. New York: John Wiley and Sons, 1981.
  6. Sun, Cheng and Walsh, T. E. “A Packaged System of a Solid-State Microwave-Biased Photoconductive Detector for 10.6 μm.” Proceedings of the IEEE 58 (October, 1970): 1732-1736.
  7. Tachibana, Akira, et al. Stereo Radar System for Automobile Collision Avoidance. Kyoto: Nissan Motor Co., Ltd., 1982.
  8. Terman, Frederick Emmons, Editor. Antennas. McGraw-Hill Electrical and Electronic Engineering Series. New York: McGraw-Hill Book Company, Inc., 1950.
  9. Terman, F. E. Radio Engineer Handbook. New York: McGraw-Hill Book Company, 1943.
  10. Third International Conference on Integrated Optics and Optical Fiber Communication 27-29 April 1981. San Francisco: Optical Society of America/Institute of Electrical and Electronic Engineers, 1981.
  11. Tomboulian, D. H. Electric and Magnetic Fields. New York: Harcourt, Brace and World, Inc., 1965.
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p. 113
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  2. Walter, Carlton H. Traveling Wave Antennas. New York: McGraw-Hill Book Company, 1975.
  3. Weissberger, Alan J. “Modems: The Key to Interfacing Digital Data to Analog Telecomm Lines.” Electronic Design 27 (10 May 1979): 82-89.
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  5. Wong, R. E., et al. Collision Avoidance Radar Braking System. Washington, D.C.: Bendix Research Laboratories, 1977.
  6. Wong, R. E., et al. Collosion Avoidance Radar Braking System Investigation - Phase II Study. Southfield, Michigan: The Bendix Corporation, 1976.
  7. Wood, L. E., Chandler, R. A., and Warren, B. D. Analysis of Problems on the Application of Radar Sensors to Automotive Collision Prevention. Boulder, Colorado: U.S. Dept. of Commerce, Office of Telecommunications, Institute for Telecommunication Sciences, 1973.
  8. Ziemer, R. E. and Tranter, W. H. Principles of Communications: Systems, Modulation, and Noise. Boston: Houghton-Mifflin Company, 1976.
p. 114

APPENDIX I: Phase Plane with Warning Boundary

p. 115
Phase Plane with Warning Boundary — range (ft) versus range-rate (ft/sec)

Phase Plane with Warning Boundary. Range (ft) versus range-rate (ft/sec), showing the warning boundary curve.

p. 116

APPENDIX II: Block Diagram of Radar Sensor

p. 117
Block Diagram of Radar Sensor

Block Diagram of Radar Sensor. The doppler transceiver (parabolic antenna with radome → circulator, Gunn oscillator at 36 GHz / 25 mW, FM pulse modulator, mixer detector) feeds a preamplifier, Ch. 1 / Ch. 2 gates, doppler amplifier limiters, and the range-rate, range, and approach-recede detectors (outputs Ṙ, R, Δ/R). A +12 V voltage regulator supplies +10.5 V and +5.0 V. A confidence monitor and a threshold channel (amplitude comparator → freq gate) provide the raw-doppler, TF, and doppler-count outputs.

p. 118

APPENDIX III: Range Calibration for Ford Granada

p. 119
Range Calibration for Ford Granada — analog range (mV) versus range (feet)

Range Calibration for Ford Granada. Analog range output (mV) versus actual range (feet). The response is approximately linear up to ~225 feet, then rolls over near 250 feet.

p. 120

APPENDIX IV: Data Documentation Technique

p. 121
Data Documentation Technique

Data Documentation Technique. Data acquisition (in the automobile): a TV camera captures the pan view; the radar sensor (RDR SNSR) and radar processor (RDR PRCSR) supply closure rate, range, speed, and warn signals (plus steering angle, vehicle speed, and braking command) to the telemetry transmitter (TELEM XMTR), with a calibrator (CALIB); video and encoded telemetry are recorded by the VTR. Data analysis (laboratory/studio): the VTP feeds a studio switcher and TV; the telemetry receiver (TELEM RCVR) and display drive a TV camera, producing the composite driving sequences.

p. 122

APPENDIX V: Telemetry Signals

p. 123

TELEMETRY TRANSMITTER SIGNALS

Function XTAL Freq (Hz.) Divide By U4 Output Pin Output Freq. (Hz.) Comments
Speed 268,800 256 13 16.2 KΩ .039 μf 100VDC 5.11 KΩ 1050.0
Range 216,960 256 13 16.2 KΩ .047 μf 100VDC 6.19 KΩ 847.5
Closure Rate 392,704 512 12 18.0 KΩ .047 μf 100VDC 3.48 KΩ 767.0
Slave 387,072 1024 14 16.2 KΩ .1 μf 16VDC 348 KΩ 378.0 SAFE
Slave 398,336 1024 14 16.2 KΩ .1 μf 16VDC 348 KΩ 389.0 WARNING

Notes: All resistors: 1/4 watt, ±1% tolerance. All capacitors: ±10% tolerance.

p. 124

AUTOMOBILE RADAR / TELEMETRY INTERFACE

Function Automobile — Color Code Automobile — Pin No. Telemetry — Color Code Telemetry — Pin No.
Speed Violet 1 White 1
Closure Rate Orange 2 Orange 2
System Ground Grey 3 Black 3
Range Green 4 Green 4
−5VDC Power Blue
Alarm Brown 5 Brown 5
−15VDC Power Yellow 7 Blue 7
+15VDC Power Red 8 Red 8
p. 125

APPENDIX VI: Telemetry Transmitter Schematics

p. 126
Transmitter — Input Isolation and Signal Conditioning (DC) Amplifier schematic

Transmitter, Input Isolation and Signal Conditioning (DC) Amplifier. Input color-code lines (brown/alarm, black, white, blue −15VDC, orange, green, red +15VDC) feed dual op-amps U1A, U2A, U2B, U1B (LM 747CN) with 5KΩ LIN pots, 1 MegΩ and 464 KΩ resistors, producing the speed, closure-rate, range, and slave/alarm transmitter inputs (each via 10 KΩ and 2.2 μf / 35VDC). Notes: all resistors 1/4 watt, ±1% tolerance; all capacitors ±10% tolerance; U1 and U2 LM 747CN integrated circuits.

p. 127
Transmitter — Precision AF Signal Generation schematic

Transmitter, Precision AF Signal Generation (one each used for speed, closure rate, and range functions). A crystal-controlled oscillator (U3A, 10 MegΩ feedback, 68 pf SM caps) drives CMOS counter U4 (MC14040AL); the divided square wave is amplitude-modulated by Q1 (2N2222) and filtered by the three-stage low-pass network (U3C, U3B; , ) to the output mixer. Notes: U3 = MC14007AL, U4 = MC14040AL CMOS; , counter output pin, and XTAL per Telemetry Transmitter Signals chart.

p. 128
Transmitter — Precision AF Signal Generation (Slave/Alarm) schematic

Transmitter, Precision AF Signal Generation (one used for slave/alarm function). Same topology as the speed/closure-rate/range generator (crystal oscillator U3A → CMOS counter U4 → modulator Q1 → three-stage LPF → output mixer), with additional connections “C” and “D” routed to the FSK section. Notes: U3 = MC14007AL, U4 = MC14040AL CMOS; Q1 = 2N2222; values per Telemetry Transmitter Signals chart.

p. 129
Transmitter — FSK and Output Summer schematic

Transmitter, FSK and Output Summer. The FSK section switches between XTAL 1 (398,336 Hz) and XTAL 2 (387,072 Hz) via 1N4148 steering diodes and transistor Q2 (2N2222), driven by the FSK input and connections “C”/“D”. The output summer combines the AF signals (with AM data) through 33 KΩ resistors to the video camera audio channel. Powered by +9VDC and a +7.5VDC “C”-battery stack. Notes: all resistors 1/4 watt ±1%; all capacitors ±10%; Q2 = 2N2222.

p. 130

APPENDIX VII: Telemetry Receiver Schematics

p. 131
Receiver — Input Amplifier schematic

Receiver, Input Amplifier. The composite audio input passes through a 20 KΩ LIN level control and 619 KΩ / 2.2 μf coupling into op-amp U1 (LM 741CN) with 422 KΩ feedback, then via 1 μf / 196 KΩ to a signal-distribution network of four 316 KΩ resistors feeding the channel amplifiers. Notes: all resistors 1/4 watt ±1%; all capacitors ±10%; U1 = LM 741CN single op amp.

p. 132
Receiver — Channel Amplifier (speed and range) schematic

Receiver, Channel Amplifier (one each used for speed and range functions). Input from the Input Amplifier feeds Microfork filter MF1 (316 KΩ / 10 MegΩ termination), an impedance buffer and gain stage (U2A, U2B — LM 747CN; 680 KΩ and 348 KΩ feedback), a half-wave voltage-doubling detector (1N270 germanium diodes), offset/gain stages (U3A, U3B with 100 KΩ LIN pots), and an output meter (100 μa, 200 μf / 3VDC). Notes: all resistors 1/4 watt ±1%; all capacitors ±10%; U2, U3 = LM 747CN dual op amp.

p. 133
Receiver — Channel Amplifier, Closure Rate schematic

Receiver, Channel Amplifier, Closure Rate. Same topology as the speed/range channel amplifier (MF1 Microfork, U2A/U2B gain stages, 1N270 doubling detector, U3A/U3B offset and gain), with an added range switch SW1 (287 KΩ / 121 KΩ) selecting display scale — position “A” = 30 m/sec, position “B” = 50 m/sec. Notes: all resistors 1/4 watt ±1%; all capacitors ±10%; U2, U3 = LM 747CN dual op amp; SW1 shown in position “A”.

p. 134
Receiver — Channel Amplifier, Warning Alarm schematic

Receiver, Channel Amplifier, Warning Alarm. The warning channel mirrors the other channel amplifiers up to the doubling detector, then feeds a gain stage (U4, LM 741CN) and a voltage comparator (U5, LM 311N) whose switched output drives an incandescent warning lamp (1819) and a Sonalert SC 628 audible alarm. Notes: all resistors except where noted 1/4 watt ±1%; all capacitors ±10%; U2 = LM 747CN dual op amp, U4 = LM 741CN single op amp, U5 = LM 311N comparator.

p. 135
Receiver — Power Supply schematic

Receiver, Power Supply. A SOLA Cat. No. 84-12-02112E supply (±12 VDC, 120 mA) provides the +12 VDC and −12 VDC rails, fed through a 1 A SB fuse and power switch, with an NE 51 neon pilot lamp (47 KΩ).

p. 136

APPENDIX VIII: Telemetry Calibrator

p. 137
Telemetry Calibrator schematic

Telemetry Calibrator. Two 1.5 V primary cells (, ) and pushbutton switches (, ) supply known reference levels through the color-coded interface lines — red (+15.0V), blue (−15.0V), brown (alarm), white (speed), green (range), orange (closure rate), black (gnd) — with test jacks for verification. Notes: (1) and pushbutton switches shown in “up” position; (2) and are primary Alkaline-Manganese Dioxide batteries, cell designation No. 315 (ANSI “L 40”).

p. 138

APPENDIX IX: Microstrip Fed Horn Antenna Suitable for AGM

p. 139
Microstrip Fed Horn Antenna Suitable for AGM — finite-element grid

Microstrip Fed Horn Antenna Suitable for AGM. The triangular wire-fed horn modeled as a finite-element grid, with the single-point feed at the apex (Y axis) and the loaded segments labeled J through X along the conduction plane. Grid cells are 0.075 wavelength; the feed region detail is 0.1 wavelength.

p. 140

APPENDIX X: Unloaded Horn

p. 141
Unloaded Horn radiation pattern (polar)

Unloaded Horn. Computed polar radiation pattern (AMP) of the unloaded Mini Pharaoh horn, showing a single forward main lobe with 3.0 dB, 6.0 dB, and 9.0 dB contours and 100% efficiency at boresight.

p. 142

APPENDIX XI: Loaded Horn

p. 143
Loaded Horn radiation pattern (polar)

Loaded Horn. Computed polar radiation pattern (AMP) of the resistively loaded Mini Pharaoh horn. Compared with the unloaded case, the beam is steered off-center and a back lobe appears; maximum gain (12.12 dB) occurs off boresight, with a slight efficiency loss (91.36%).

p. 144

APPENDIX XII: Semiconductor Energy Diagram

p. 145
Semiconductor Energy Diagram

Semiconductor Energy Diagram. Energy-band model showing the conduction band and valence band separated by the band gap , with the donor level and acceptor level within the gap. Arrows indicate the three optical excitation transitions (donor→conduction, valence→acceptor, and valence→conduction electron-hole pair generation).

p. 146

APPENDIX XIII: Type 4, CdSe Typical Resistance vs. Illumination Characteristics

p. 147
Type 4 CdSe — typical resistance versus illumination characteristics

Type 4, CdSe — Typical resistance vs. illumination characteristics. Log-log family of curves (A through H) for different device geometries, plotting cell resistance (ohms, 10 Ω to 1 MΩ) against illumination (0.01 to 100 foot-candles). Resistance falls roughly two to three decades from darkness to full illumination.

p. 148

APPENDIX XIV: Variation of Conductance with Light History

p. 149
Variation of Conductance with Light History

Variation of Conductance with Light History (CdSe material). Ratio of conductances versus illumination (foot-candles) for Type 3 and Type 4 material, where = conductivity measured from infinite dark history and = conductivity measured from infinite 30 ft-c light history. Type 4 shows a markedly smaller light-history effect than Type 3.

p. 150

APPENDIX XV: Minimum Search Time Determination (RF Considerations)

p. 151

The basic radar equation is given as follows:

where - = received power - = transmitted power - = gain of the transmitting antenna - = range - = radar cross section of the target - = effective area of the receiving antenna

Assuming coherent detection, the minimum detectable signal is calculated:

where - = detection index (after Peterson and Birdsall, as per reference 79) - = receiver noise figure - = Boltzman’s constant ( watt-seconds/degree) - = 290 degrees Kelvin (The input noise is usually . If not, must be replaced by actual noise out of the receiver divided by its total cascaded gain.) - = bandwidth - = transmitted pulse duration ( is the coherent processing gain)

p. 152

Let , then,

where = maximum system range

The total energy transmitted per pulse is:

Thus, EQ III becomes:

The solid angle covered by each pulse may be related approximately to the gain of the antenna by . The total solid angle covered in seconds is therefore [79]:

where - = search time - = number of pulses per second

Rearranging EQ VI:

Substituting EQ VII (G) into EQ V:

but,

p. 153

where = average radar power,

so,

Rearranging terms:

accounting for system efficiency ():

p. 154

APPENDIX XVI: Type 4, CdSe Peak Spectral Response 690.0 Nanometers

p. 155
Type 4 CdSe peak spectral response, 690.0 nanometers

Type 4, CdSe — Peak spectral response, 690.0 nanometers. Normalized sensitivity (%) versus wavelength (nanometers). Response rises gradually from ~400 nm, peaks sharply near 690 nm (red), then falls off toward 1000 nm.

p. 156

APPENDIX XVII: LED Optical Output Characteristic

p. 157
LED Optical Output Characteristic

LED Optical Output Characteristic. Relative emission intensity of the GaAlAs LED versus wavelength (nanometers). The output is a narrow band peaking near 660 nm, closely overlapping the CdSe spectral-response peak (690 nm).

p. 158

APPENDIX XVIII: LED Transfer Characteristic

p. 159
LED Transfer Characteristic

LED Transfer Characteristic. Relative luminous intensity versus LED forward current (, mA). Output is strongly nonlinear — near zero below ~5 mA, then rising approximately linearly to ~2.4 at 40 mA.

p. 160

APPENDIX XIX: Equivalent Microwave Circuits

p. 161
Equivalent Microwave Circuits — Figures 1–4

Equivalent Microwave Circuits. Fig. 1 — Serpentine microwave capacitor “” (interdigitated layout, terminals 1–2). Fig. 2 — Serpentine microwave capacitor “” equivalent circuit (distributed inductors and capacitors). Fig. 3 — Serpentine microwave capacitor with inductive shunt on the reverse side of the substrate (shunt / substrate / Indium cross-section, terminals 3–4). Fig. 4 — Equivalent circuit model of the shunted device, showing the crossed distributed coupling around “”.

p. 162

APPENDIX XX: Microwave Photoconductive Element

p. 163
Microwave Photoconductive Element — top and side views with dimensions

Microwave Photoconductive Element. Top view: a CdSe channel (0.006 in. wide Indium gap) runs between two end holes spaced 0.195 in. center-to-center (each hole 0.026 in.), with connection-bond pads on either side; overall width 0.223 in. Side view: the Al₂O₃ substrate is 0.263 in. long and 0.040 in. thick.

p. 164

APPENDIX XXI: Microwave Photoconductive Element Models

p. 165
Microwave Photoconductive Element Models — networks A, B, C

Microwave Photoconductive Element Models. (A) The full network: two end inductors (L), the coplanar capacitor (C), and the photoconductor (variable R) in parallel. (B) The two end inductors combined into an equivalent L/2 in parallel with C and R. (C) At resonance the reactances cancel and the device reduces to pure resistance R.

p. 166

APPENDIX XXII: Geometric Model used in Determining Total (Untuned) Device Capacitance

p. 167
Geometric Model used in Determining Total (Untuned) Device Capacitance

Geometric Model used in Determining Total (Untuned) Device Capacitance. Cross section of the microwave photoconductor (CdSe channel between Indium contacts on an Al₂O₃ substrate) showing the capacitance contributions: (total field confinement region within the substrate), (free-space flux on one side), (parallel-plate regions inside the substrate), and (free-space flux linking the two capacitors).

p. 168

APPENDIX XXIII: Total Device Capacitance Calculations

p. 169

Total Device Capacitance Calculations

where and are complete elliptic integrals of the first kind

and farads/inch

and = length = 0.195 − 0.026 = 0.169 inches

where A = plate area = wh, w = plate width

Therefore,

Now,

so,

p. 170

Thus,

Now,

Calculate :

Find :

Compute total device capacitance:

p. 171

APPENDIX XXIV: Microwave Photoconductive Element with Tuner

p. 172
Microwave Photoconductive Element with Tuner

Microwave Photoconductive Element with Tuner. Top view of the device showing the brass tuning strips (dashed) positioned diagonally across the reverse side of the substrate to alter device capacitance and inductance, tuning the resonant frequency after Indium deposition.

p. 173

APPENDIX XXV: SMA Test Fixture Performance

p. 174
SMA Test Fixture Performance with blank conductive chip

SMA Test Fixture Performance with Blank Conductive Chip (channel spacing = .25″, = 0.4 Ω). Transmission stays near −6 to −8 dB across 8–12.4 GHz; isolation > 50 dB. (“NO DOT END” annotations appear above and below the isolation baseline.)

p. 175
SMA Test Fixture Performance with blank conductive chip (dot end)

SMA Test Fixture Performance with Blank Conductive Chip (channel spacing = .25″, DOT END side, = 1.2 Ω). Transmission for the second fixture position stays near −6 to −9 dB across 8–12.4 GHz; isolation > 50 dB.

p. 176
SMA Test Fixture Performance with cylindrical conductor

SMA Test Fixture Performance with Cylindrical Conductor (center conductor diameter = .0159″, channel spacing = .25″). Replacing the blank chip with a cylindrical conductor greatly affects the transmission characteristics — transmission ranges roughly −6 to −13 dB across 8–12 GHz with wide excursions for small frequency shifts; isolation > 50 dB.

p. 177
SMA Test Fixture Performance with cylindrical conductor (dot end)

SMA Test Fixture Performance with Cylindrical Conductor (center conductor diameter = .0159″, channel spacing = .25″, DOT END side). The second fixture position again shows wide transmission excursions (roughly −5 to −13 dB) across 8–12.4 GHz; isolation > 50 dB.

p. 178

APPENDIX XXVI: Mini Pharaoh Radiation Pattern

p. 179
Mini Pharaoh Radiation Pattern (polar)

Mini Pharaoh Radiation Pattern. Computed polar radiation pattern (AMP) of a single Mini Pharaoh horn (1.4 wavelength leading edge), showing a single forward main lobe with 3, 6, 9, and 12 dB contours and a forward gain of 12.64 dB above an isotropic radiator.

p. 180

APPENDIX XXVII: Isotropic Sources Spaced 3λ/2

p. 181
Isotropic Sources Spaced 3λ/2 — array factor pattern (polar)

Isotropic Sources Spaced 3λ/2. Polar plot of the array factor for two in-phase isotropic radiators spaced 1.5 wavelengths apart, showing the multi-lobe pattern (contours at 1.5, 3.0, 4.5, and 6.0 dB) with the main beam broadside to the line joining the sources.

p. 182

APPENDIX XXVIII: Bihorn Radiation Pattern

p. 183
Bihorn Radiation Pattern (polar)

Bihorn Radiation Pattern. Computed polar radiation pattern (AMP) of the two-element Mini Pharaoh bihorn array with in-phase excitation, showing the forward main lobe (broadside, ~180°), symmetric side lobes, and a rear lobe, with contours at 4, 8, 12, and 16 dB.

p. 184

APPENDIX XXIX: Antenna RF Configuration

p. 185
Antenna RF Configuration

Antenna RF Configuration. The bihorn — two microstrip radiators (each 1.4 λ, spaced 1.5 λ) fed by a common phasing line — connects through the microwave photoconductive elements and ferrite isolators (50 Ω circulators) to a Wilkinson power divider, driven by the Gunn source (with power and varactor-tune connections).

p. 186

APPENDIX XXX: Schematic Diagram of Microwave Transmitter

p. 187
Schematic Diagram of Microwave Transmitter — Power Supply

Power Supply, Microwave Transmitter. A line transformer (Signal 241-7-36) and 1N5408/1N4007 rectifier bank feed two LM317 regulators producing +15 VDC rails (with +19 VDC intermediate). LED current steering uses 1 KΩ LIN controls and dual analog meters (20 mA right/left), and 15 V D.C. power is supplied to the modulator. An NE51 neon pilot lamp and a 9-pin connector complete the unit. Notes: resistors 1/4 watt ±1%; all capacitors ±10% tolerance.

p. 188
Schematic Diagram of Microwave Transmitter — Modulator

Modulator, Microwave Transmitter. A CMOS ICM7555 timer (with 100 KΩ LIN frequency control) generates the square-wave modulation; a complementary-symmetry pulse amplifier (2N6049 / 2N3054A output transistors driven by 2N2222 stages) produces the MOD OUT pulse to the Gunn source. Powered from the +15 V / +10 V D.C. supply. Notes: resistors 1/4 watt ±1%; all capacitors ±10% tolerance.

p. 189

APPENDIX XXXI: Bihorn Phasor Calculations (Amplitude to Phase Conversion)

p. 190

Bihorn Phasor Calculations (Amplitude to Phase Conversion)

(electrical spacing of feed points) = 137.8°

Steer on Boresight:

Phasor 1:

Phasor 2:

Steer Full Right:

Phasor 1:

Phasor 2:

p. 191

Steer Full Left:

Phasor 1:

Phasor 2:

Thus

p. 192

APPENDIX XXXII: Inductance Formula Sensitivity Analysis

p. 193

Inductance Formula Sensitivity Analysis

The Dukes inductance formula is given for a flat single turn circular conducting loop:

where - is in nanohenries - = outer circumference in mils - = loop width in mils - = loop thickness in mils

for

but

where = outer radius in mils, = inner radius in mils

therefore,

define:

therefore,

p. 194

Since the inner radius () is held constant (the hole size), the following is noted:

The inductance (L) is proportional to y.

define:

or,

examine y.

Let

and

or

also, rearranging EQ VIII:

so,

or,

p. 195

or,

or,

or,

It is noted that is extremely small for values of above ~2. In fact, for . The almost horizontal slopes demonstrate that the predicted values of inductance have low dependency on in these regions. In sections 4.3.2 of the text two cases were cited:

Case A (Minimum Width)

= 13 mils, = 34 mils

= 21 mils

therefore,

thus,

p. 196

recall EQ VI:

or,

or,

or,

substituting for :

or,

Clearly, this is a very small inductance rate of change.

Case B (Double Width)

mils, mils

mils

therefore,

thus,

p. 197

or,

Again, a very small inductance rate of change is noted. Included on the following page is a plot of y versus . Also indicated on the vertical axis are corresponding inductance values. Note mils.

p. 198
Inductance versus α (r₁ = 0.013 in.)

Inductance versus α ( = 0.013 in.). Plot of (and corresponding inductance in nH) against . The curve falls steeply then flattens; markers indicate Case A (), the zero-slope point (, slope = 0), and Case B (), confirming the low dependence of inductance on in this region.

p. 199

APPENDIX XXXIII: Demonstration Equipment Photographs

p. 200
Fig. 1 — Microwave Photoconductive Element (photograph)

Fig. 1. Microwave Photoconductive Element. Photograph of a fabricated device shown resting on a U.S. penny for scale, illustrating the small size of the CdSe element with its two end holes and channel.

p. 201
Fig. 2 — Antenna and RF Components (photograph)

Fig. 2. Antenna and RF Components. Photograph of the assembled bihorn radiating structure with its phasing line, microwave photoconductive elements, and associated RF components mounted on a wooden test stand.

p. 202
Fig. 3 — Microwave Transmitter Control Unit (photograph)

Fig. 3. Microwave Transmitter Control Unit. Photograph of the control panel showing the two Western Electric milliampere meters (LED 1 and LED 2 current monitors), the LED current-steering controls, and the LED OFF / PWR ON switches.

p. 203
Fig. 4 — Receiving Horn with Frequency Meter (photograph)

Fig. 4. Receiving Horn with Frequency Meter. Photograph of the pyramidal receiving horn antenna with its waveguide end-short cavity and crystal rectifier, mounted on the adjustable stand-off tower used during system testing.

  1. vita

VITA

Vincent Paul McGinn was born in The Bronx, New York City. Following graduation from Mt. St. Michael Academy he attended New York University. Here he received a bachelor of engineering (in electrical engineering) degree and a master of science (in electrical engineering) degree. He has also been awarded a master of science degree in astronomy from The Pennsylvania State University. Dr. McGinn is a registered professional engineer.


  1. Operation of a radar at high frequencies (like 36 Gigahertz) is afflicted with backscatter from rain. Circular polarization can minimize this effect.↩︎

  2. E-Solder 3021 Conductive Adhesives, Acme Chemicals and Insulation Co., Division of Allied Products Corporation, New Haven, Connecticut 06505↩︎

  3. E-POX-E Stock No. EPX-5, Duro, Woodhill Chemical Sales, Cleveland, Ohio 44128↩︎

  4. Model FS-1371, Frequency Sources, Inc., Chelmsford, Massachusetts 01824↩︎

  5. Model 8821, Norsal Industries, Central Islip, New York 11722↩︎

  6. Part No. 1420-1920, Trak Microwave Corporation, Tampa, Florida 33614↩︎

  7. Literature searches accomplished (domestic and foreign) by Dialog Information Services, Inc., 3460 Hillview Avenue, Palo Alto, California 94304↩︎