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An Efficient Propagation Simulator for High Frequency Signals And Results from HF radar experiment. Kin Shing Bobby Yau Supervisors: Dr. Chris Coleman & Dr. Bruce Davis School of Electrical and Electronic Engineering The University of Adelaide, Australia. Overview.
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An Efficient Propagation Simulator for High Frequency SignalsAnd Results from HF radar experiment Kin Shing Bobby Yau Supervisors: Dr. Chris Coleman & Dr. Bruce Davis School of Electrical and Electronic Engineering The University of Adelaide, Australia
Overview • HF Ionospheric Propagation Simulator • Simulation results • Comparisons with Experimental Results • Discussions • Conclusions
Introduction HF radio system is still prevalent • Military Over-the-Horizon RADAR • HF communications • Commercial broadcasting
Ionospheric Propagation Simulator • A need for wideband HF propagation simulator • Focussing on the fading effects of HF signals • Employ theoretical model of fading • Efficient algorithm based on analytical expressions • Two components of fading model: • Polarization Fading Model • Amplitude Fading Model
Polarization Fading Model • Faraday rotation due to O and X wave interference
Polarization Fading Model • Perturbation techniques to ascertain the change in phase path due to irregularities • Use of frequency offset method to take into account of the magnetic field
Amplitude Fading Model • Focussing and defocussing of radio waves due to movement of large scale ionospheric structure
Amplitude Fading Model • Parabolic approximation to Maxwell’s equation (Wagen and Yeh): • U is the complex amplitude, is the refractive index with irregularities • g and t are the local longitudinal and transverse coordinates
Simulator Implementation • Numerical ray tracing is used for the path quantities • Accurate ray homing for finding all possible paths (Strangeways, 2000) • Fading is calculated by the fading models
Simulation Results • Alice Springs to Darwin
Simulation Results • 10.6MHz - = 0.05, L = 350km, v = 200m/s
Simulation Results • 10.6MHz - = 0.05, L = 350km, v = 200m/s
Simulation Results • 10.6MHz - = 0.05, L = 350km, v = 200m/s
Simulation Results • 10.6MHz - = 0.20, L = 350km, v = 200m/s
Simulation Results • 10.6MHz - = 0.20, L = 350km, v = 200m/s
Simulation Results • 10.6MHz - = 0.20, L = 350km, v = 200m/s
Comparison – Experimental Results • Signals from Jindalee Radar transmitter in Alice Springs • Dual-polarization receiver in Darwin
FMCW Radar signal Experimental Results Finding the signal component along each sweep
6:30PM local time – Spectrograms Experimental Results
6:30PM local time – Time fading Experimental Results
6:30PM local time – Frequency fading Experimental Results
7:30PM local time – Spectrograms Experimental Results
7:30PM local time – Time fading Experimental Results
7:30PM local time – Frequency fading Experimental Results
Fading Separation • Separate amplitude and polarisation fading • Two orthogonal antennas: • A - amplitude component - phase component • Therefore:
7:30PM local time – Time fading revisited Fading Separation
7:30PM local time – Time fading separation Fading Separation
6:30PM local time – Time fading revisited Fading Separation
6:30PM local time – Time fading separation Fading Separation
Fading Separation • Fading separation works well for single-mode case • For multi-mode propagation: • Exploit FMCW radar signals • Separating the modes using Range-gating techniques • Applying fade separation to each of the modes
Discussion • Further analyzing with experimental data • Comparisons with ionosonde data • Discover the structure of the ionosphere during the period of rapid fading • Simulating propagation under realistic irregularity strctures • Possible applications: • Real-Time channel evaluation • Test-bed for fading mitigation techniques
Conclusion • Efficient Ionospheric Propagation Simulator has been developed • Experiment to observe fading of HF signals was done successfully • Comparisons between experiment and simulation are promising, especially for single-path polarization fading • More work to be done on the experimental data
Acknowledgements • Defence Science and Technology Organisation (DSTO) • Dr. Manuel Cevira • Dr. Chris Coleman