Conjuring Radar Meteor Head-Echoes

John David Mathews

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The argument surrounding under-dense vs. over-dense radar meteors has raged for decades. Here we consider the head-echo case by the noting that the two limiting scattering regimes for the same radar scattering cross-section (RCS) are each easily described. We give a synopsis of scattering from a perfectly conducting (PC) sphere that represents the manifestly over-dense limit. We contrast this with coherent (in-phase) scattering from an ensemble of N electrons all located within a and sim;1/4-wavelength diameter volume containing the meteoroid. Note that N is the absolute minimum number of electrons yielding a given RCS and that the continuum of equal RCS electron distributions leading to the PC-sphere all require more electrons and thus higher energy to assemble. Here we find the loci of equal RCS for these two limiting cases at three wavelengths - 70 cm, 1.29 m, and 6 m - corresponding to the Arecibo Observatory (AO), EISCAT-3D, and Jicamarca Radio Observatory (JRO) radars, respectively. We also plot on each of these curves the location of a single-pulse (unaveraged), 100 km range, SNR=1 event. In all cases the over-dense (Rayleigh scatter) meteor would correspond to an improbably large object while the number of electrons, N, yielding the same RCS is reasonable. Invoking Occam's Razor, we conclude that the vast majority of head-echo radar meteors are under-dense. This conclusion is important to many aspects of meteoroid physics including mass flux determinations as N is relatively easy to link to meteoroid physics and thus to meteoroid mass. This remains largely true when meteoroid inhomogeneity and fragmentation are considered.

Original languageEnglish (US)
Title of host publication2018 2nd URSI Atlantic Radio Science Meeting, AT-RASC 2018
PublisherInstitute of Electrical and Electronics Engineers Inc.
ISBN (Electronic)9789082598735
DOIs
StatePublished - Sep 24 2018
Event2nd URSI Atlantic Radio Science Meeting, AT-RASC 2018 - Gran Canaria, Spain
Duration: May 28 2018Jun 1 2018

Other

Other2nd URSI Atlantic Radio Science Meeting, AT-RASC 2018
CountrySpain
CityGran Canaria
Period5/28/186/1/18

Fingerprint

meteoroids
radar scattering
radar
echoes
Radar
Scattering
scattering cross sections
Electrons
Observatories
observatories
Physics
scattering
N electrons
radar echoes
conduction
Wavelength
physics
electrons
loci
electron distribution

All Science Journal Classification (ASJC) codes

  • Computer Networks and Communications
  • Signal Processing
  • Electrical and Electronic Engineering
  • Instrumentation

Cite this

Mathews, J. D. (2018). Conjuring Radar Meteor Head-Echoes. In 2018 2nd URSI Atlantic Radio Science Meeting, AT-RASC 2018 [8471509] Institute of Electrical and Electronics Engineers Inc.. https://doi.org/10.23919/URSI-AT-RASC.2018.8471509
Mathews, John David. / Conjuring Radar Meteor Head-Echoes. 2018 2nd URSI Atlantic Radio Science Meeting, AT-RASC 2018. Institute of Electrical and Electronics Engineers Inc., 2018.
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Mathews, JD 2018, Conjuring Radar Meteor Head-Echoes. in 2018 2nd URSI Atlantic Radio Science Meeting, AT-RASC 2018., 8471509, Institute of Electrical and Electronics Engineers Inc., 2nd URSI Atlantic Radio Science Meeting, AT-RASC 2018, Gran Canaria, Spain, 5/28/18. https://doi.org/10.23919/URSI-AT-RASC.2018.8471509

Conjuring Radar Meteor Head-Echoes. / Mathews, John David.

2018 2nd URSI Atlantic Radio Science Meeting, AT-RASC 2018. Institute of Electrical and Electronics Engineers Inc., 2018. 8471509.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

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Mathews JD. Conjuring Radar Meteor Head-Echoes. In 2018 2nd URSI Atlantic Radio Science Meeting, AT-RASC 2018. Institute of Electrical and Electronics Engineers Inc. 2018. 8471509 https://doi.org/10.23919/URSI-AT-RASC.2018.8471509