Articles | Volume 39, issue 4
https://doi.org/10.5194/angeo-39-709-2021
https://doi.org/10.5194/angeo-39-709-2021
Regular paper
 | 
23 Jul 2021
Regular paper |  | 23 Jul 2021

Effect of neutral winds on the creation of non-specular meteor trail echoes

Freddy Galindo, Julio Urbina, and Lars Dyrud

Download

Interactive discussion

Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
Printer-friendly Version - Printer-friendly version Supplement - Supplement

Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision
ED: Publish subject to revisions (further review by editor and referees) (18 Jan 2021) by Keisuke Hosokawa
AR by Julio Urbina on behalf of the Authors (02 Mar 2021)  Author's response   Author's tracked changes   Manuscript 
ED: Referee Nomination & Report Request started (05 Mar 2021) by Keisuke Hosokawa
RR by Anonymous Referee #1 (04 Apr 2021)
ED: Publish subject to revisions (further review by editor and referees) (05 Apr 2021) by Keisuke Hosokawa
AR by Julio Urbina on behalf of the Authors (04 Jun 2021)  Author's response   Author's tracked changes   Manuscript 
ED: Publish as is (08 Jun 2021) by Keisuke Hosokawa
AR by Julio Urbina on behalf of the Authors (16 Jun 2021)  Manuscript 
Download
Short summary
Micro-size particles entering the Earth’s atmosphere do not emit enough light to be observed as meteors, but they can be probed with radars. The echo from these meteors depends on particle size and the atmosphere in which the particle travels. In this paper, we study the importance of neutral winds in forming meteor returns sensed by radars. We show that meteor trails can exhibit unique radar signatures due to neutral winds, explaining unique signatures in radar maps.