Articles | Volume 39, issue 1
https://doi.org/10.5194/angeo-39-239-2021
https://doi.org/10.5194/angeo-39-239-2021
Regular paper
 | 
25 Feb 2021
Regular paper |  | 25 Feb 2021

Statistical study of linear magnetic hole structures near Earth

Martin Volwerk, David Mautner, Cyril Simon Wedlund, Charlotte Goetz, Ferdinand Plaschke, Tomas Karlsson, Daniel Schmid, Diana Rojas-Castillo, Owen W. Roberts, and Ali Varsani

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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: Publish subject to revisions (further review by editor and referees) (11 Nov 2020) by Anna Milillo
AR by Martin Volwerk on behalf of the Authors (12 Nov 2020)  Author's response    Manuscript
ED: Referee Nomination & Report Request started (12 Nov 2020) by Anna Milillo
RR by Anonymous Referee #1 (20 Dec 2020)
RR by Anonymous Referee #2 (19 Jan 2021)
ED: Publish subject to minor revisions (review by editor) (20 Jan 2021) by Anna Milillo
AR by Svenja Lange on behalf of the Authors (22 Jan 2021)  Author's response
ED: Publish subject to technical corrections (22 Jan 2021) by Anna Milillo
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Short summary
The magnetic field in the solar wind is not constant but varies in direction and strength. One of these variations shows a strong local reduction of the magnetic field strength and is called a magnetic hole. These holes are usually an indication that there is, or has been, a temperature difference in the plasma of the solar wind, with the temperature along the magnetic field lower than perpendicular. The MMS spacecraft data have been used to study the characteristics of these holes near Earth.