Frequency shifts of head echos in meteoroid trail formation
Hans W. Wilschut

TL;DR
This paper derives the frequency shift of radar echoes from meteoroids, analyzing head echos during trail formation, and compares models to observations to understand plasma behavior.
Contribution
It introduces a theoretical framework for the frequency shifts of meteoroid radar echoes and compares models to observed data to interpret plasma dynamics.
Findings
Frequency shifts are identical in different models despite physics differences.
Calculations match qualitative features of observed echoes.
Absence of negative shifts suggests co-moving plasma in front of meteoroids.
Abstract
The approximate frequency shift of a radar echo from a meteoroid is derived. The origin of head echos observed during trail formation are discussed by considering schematic models. The echo is either a reflection of the radar signal from thermalized electrons in the meteoroid trail or from the plasma electrons co-moving with the meteoroid itself. It is shown that in these opposite models the frequency shifts of the echo relative to the radar emitter frequency must be identical, even though the underlying physics differs. Calculations were made that give the echo frequency as function of time, allowing qualitative comparison with observations. Some typical observations show a conspicuous absence of negative frequency shifts in the head echo in forward scattering. Arguments are given that this can correspond to meteoroids with the co-moving plasma in front.
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Taxonomy
TopicsIonosphere and magnetosphere dynamics · Astro and Planetary Science · Magnetic confinement fusion research
