Both high‐power large aperture radars and smaller meteor radars readily observe the dense head plasma produced as a meteoroid ablates. However, determining the mass of such meteors based on the information returned by the radar is challenging. We present a new method for deriving meteor masses from single‐frequency radar measurements, using a physics‐based plasma model and finite‐difference time‐domain (FDTD) simulations. The head plasma model derived in Dimant and Oppenheim (2017),
- Award ID(s):
- 2010890
- PAR ID:
- 10396533
- Date Published:
- Journal Name:
- Chemical Communications
- Volume:
- 57
- Issue:
- 83
- ISSN:
- 1359-7345
- Page Range / eLocation ID:
- 10931 to 10934
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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- Free Publicly Accessible Full Text
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Accepted Manuscript1.0
- Journal Article:
- https://doi.org/10.1039/D1CC04211D
