Articles | Volume 37, issue 5
https://doi.org/10.5194/angeo-37-877-2019
https://doi.org/10.5194/angeo-37-877-2019
Regular paper
 | 
24 Sep 2019
Regular paper |  | 24 Sep 2019

Low-frequency magnetic variations at the high-β Earth bow shock

Anatoli A. Petrukovich, Olga M. Chugunova, and Pavel I. Shustov

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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) (14 May 2019) by Christopher Owen
AR by Anatoli Petrukovich on behalf of the Authors (09 Jun 2019)  Author's response   Manuscript 
ED: Referee Nomination & Report Request started (19 Jun 2019) by Christopher Owen
RR by Anonymous Referee #1 (22 Jun 2019)
RR by Anonymous Referee #2 (21 Jul 2019)
ED: Publish subject to minor revisions (review by editor) (05 Aug 2019) by Christopher Owen
AR by Anatoli Petrukovich on behalf of the Authors (25 Aug 2019)  Author's response   Manuscript 
ED: Publish as is (30 Aug 2019) by Christopher Owen
AR by Anatoli Petrukovich on behalf of the Authors (02 Sep 2019)  Author's response   Manuscript 
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Short summary
Earth's bow shock in solar wind with high thermal and low magnetic pressure is a rare phenomenon. However, such an object is ubiquitous in astrophysical plasmas. We surveyed statistics of such shock observations since 1995. About 100 crossings were initially identified. In this report 22 crossings from the Cluster project were studied using multipoint analysis, which allowed for the determination of the spatial scales of the shock transition and of the dominant magnetic variations