Articles | Volume 40, issue 1
https://doi.org/10.5194/angeo-40-1-2022
https://doi.org/10.5194/angeo-40-1-2022
Regular paper
 | 
04 Jan 2022
Regular paper |  | 04 Jan 2022

Types of pulsating aurora: comparison of model and EISCAT electron density observations

Fasil Tesema, Noora Partamies, Daniel K. Whiter, and Yasunobu Ogawa

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Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on angeo-2021-16', Michael Kosch, 09 May 2021
    • AC1: 'Reply on RC1', Fasil Tesema, 25 Aug 2021
  • RC2: 'Comment on angeo-2021-16', Allison Jaynes, 28 May 2021
    • AC2: 'Reply on RC2', Fasil Tesema, 25 Aug 2021

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision
ED: Publish subject to revisions (further review by editor and referees) (08 Sep 2021) by Dalia Buresova
AR by Fasil Tesema on behalf of the Authors (08 Sep 2021)  Author's response    Manuscript
ED: Referee Nomination & Report Request started (24 Sep 2021) by Dalia Buresova
ED: Publish subject to minor revisions (review by editor) (15 Oct 2021) by Dalia Buresova
AR by Fasil Tesema on behalf of the Authors (15 Nov 2021)  Author's response    Manuscript
ED: Publish as is (22 Nov 2021) by Dalia Buresova
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Short summary
In this study, we present the comparison between an auroral model and EISCAT radar electron densities during pulsating aurorae. We test whether an overpassing satellite measurement of the average energy spectrum is a reasonable estimate for pulsating aurora electron precipitation. When patchy pulsating aurora is dominant in the morning sector, the overpass-averaged spectrum is found to be a reasonable estimate – but not when there is a mix of pulsating aurora types in the post-midnight sector.