We present results and analysis of finite‐difference time‐domain (FDTD) simulations of electromagnetic waves scattering off meteor head plasma using an analytical model and a simulation‐derived model of the head plasma distribution. The analytical model was developed by (Dimant & Oppenheim, 2017b,
Obtaining meteoroid mass from head echo radar cross section depends on the assumed plasma density distribution around the meteoroid. An analytical model presented in Dimant and Oppenheim (2017a,
- Award ID(s):
- 1755020
- PAR ID:
- 10460200
- Publisher / Repository:
- DOI PREFIX: 10.1029
- Date Published:
- Journal Name:
- Journal of Geophysical Research: Space Physics
- Volume:
- 124
- Issue:
- 5
- ISSN:
- 2169-9380
- Page Range / eLocation ID:
- p. 3810-3826
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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