Articles | Volume 36, issue 5
https://doi.org/10.5194/angeo-36-1361-2018
https://doi.org/10.5194/angeo-36-1361-2018
Regular paper
 | 
17 Oct 2018
Regular paper |  | 17 Oct 2018

Characteristics of the electrojet during intense magnetic disturbances

Liudmila I. Gromova, Matthias Förster, Yakov I. Feldstein, and Patricia Ritter

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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) (31 Aug 2018) by Elias Roussos
AR by Anna Mirena Feist-Polner on behalf of the Authors (10 Sep 2018)  Author's response
ED: Referee Nomination & Report Request started (13 Sep 2018) by Elias Roussos
RR by Anonymous Referee #1 (14 Sep 2018)
RR by Anonymous Referee #2 (20 Sep 2018)
ED: Publish subject to minor revisions (review by editor) (20 Sep 2018) by Elias Roussos
AR by Matthias Förster on behalf of the Authors (30 Sep 2018)  Author's response    Manuscript
ED: Publish as is (04 Oct 2018) by Elias Roussos
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Short summary
Hall current variations in different time sectors during six magnetic storms of the summer seasons in 2003 and 2005 are examined. The sequence of the phenomena, their structure, positions and the strength of the polar and the auroral Hall electrojets were investigated using scalar magnetic field measurements obtained from the CHAMP satellite. We analyzed the correlations and the regression relations of the electrojets with auroral and ring current activity, the IMF, and solar wind parameters.