1974
DOI: 10.1109/proc.1974.9666
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Complex space-time rays and their application to pulse propagation in lossy dispersive media

Abstract: Abmct-kymptotic transient field mlutions of the form A(r, t ) exp [is@, r)] , where S is a rapidly and A a slowly varying function of space and time, may be analyzed in terms of wave packets with c e n e frequency w = -as/at and central wavenumber f = VS. When the (dis-@e) medium is lodes, stationary, and homogeneous, wave packets with constant real w aud k move dong straightline trajectories called space-time rays. In the presence of dissipation and (or) when the input signal has an exponential amplitude depe… Show more

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Cited by 50 publications
(18 citation statements)
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“…The pulse envelope spectrum , modulation frequency distribution , original and modified propagation relations and , and waveguide transfer function were all computed directly from (41), (14), (1), (17), and (2), respectively, on the sampled values. The spectrum of the waveguide excitation signal at the target was computed as in (15) with discrete convolution using the truncated envelope .…”
Section: Simulation and Numeric Resultsmentioning
confidence: 99%
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“…The pulse envelope spectrum , modulation frequency distribution , original and modified propagation relations and , and waveguide transfer function were all computed directly from (41), (14), (1), (17), and (2), respectively, on the sampled values. The spectrum of the waveguide excitation signal at the target was computed as in (15) with discrete convolution using the truncated envelope .…”
Section: Simulation and Numeric Resultsmentioning
confidence: 99%
“…The derivative of (7) with respect to defines and the derivative of (3) with respect to defines . Applying the chain rule and substituting (3) for yields the modulation frequency distribution (14) Note that, while depends upon spatial location, the dependence cancels out of the relation in (14).…”
Section: ) Pulse Distribution Functionmentioning
confidence: 99%
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