Articles | Volume 39, issue 6
Ann. Geophys., 39, 975–989, 2021
https://doi.org/10.5194/angeo-39-975-2021
Ann. Geophys., 39, 975–989, 2021
https://doi.org/10.5194/angeo-39-975-2021

Regular paper 25 Nov 2021

Regular paper | 25 Nov 2021

Fine-scale dynamics of fragmented aurora-like emissions

Daniel K. Whiter et al.

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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-2020-95', Michael Kosch, 29 Apr 2021
    • AC1: 'Reply on RC1', Daniel Whiter, 19 Aug 2021
  • RC2: 'Comment on angeo-2020-95', Anonymous Referee #2, 08 Jun 2021
    • AC2: 'Reply on RC2', Daniel Whiter, 19 Aug 2021

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision
ED: Publish as is (19 Aug 2021) by Steve Milan
AR by Daniel Whiter on behalf of the Authors (20 Aug 2021)  Author's response
ED: Publish as is (20 Oct 2021) by Steve Milan
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Short summary
This paper presents an analysis of high-resolution optical and radar observations of a phenomenon called fragmented aurora-like emissions (FAEs) observed close to aurora in the high Arctic. The observations suggest that FAEs are not caused by high-energy electrons or protons entering the atmosphere along Earth's magnetic field and are, therefore, not aurora. The speeds of the FAEs and their internal dynamics were measured and used to evaluate theories for how the FAEs are produced.