Articles | Volume 36, issue 3
https://doi.org/10.5194/angeo-36-891-2018
https://doi.org/10.5194/angeo-36-891-2018
Regular paper
 | 
20 Jun 2018
Regular paper |  | 20 Jun 2018

Differentiating diffuse auroras based on phenomenology

Eric Grono and Eric Donovan

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Interactive discussion

Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
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Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision
ED: Reconsider after major revisions (further review by editor and referees) (25 Apr 2018) by Yoshizumi Miyoshi
AR by Eric Grono on behalf of the Authors (02 May 2018)  Author's response    Manuscript
ED: Referee Nomination & Report Request started (04 May 2018) by Yoshizumi Miyoshi
RR by Anonymous Referee #1 (16 May 2018)
RR by Anonymous Referee #2 (31 May 2018)
ED: Publish as is (04 Jun 2018) by Yoshizumi Miyoshi
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Short summary
The solar wind reshapes Earth's magnetic field to create our magnetosphere and powers many dynamic processes in our plasma-filled environment, some of which produce the aurora. Networks of ground-based all-sky cameras are valuable tools that offer a large field-of-view with which to study the aurora. Using sequences of auroral images, this study defines criteria for differentiating an important type of aurora whose subcategories are often conflated.