Articles | Volume 38, issue 3
https://doi.org/10.5194/angeo-38-683-2020
https://doi.org/10.5194/angeo-38-683-2020
Regular paper
 | 
09 Jun 2020
Regular paper |  | 09 Jun 2020

Outer radiation belt and inner magnetospheric response to sheath regions of coronal mass ejections: a statistical analysis

Milla M. H. Kalliokoski, Emilia K. J. Kilpua, Adnane Osmane, Drew L. Turner, Allison N. Jaynes, Lucile Turc, Harriet George, and Minna Palmroth

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AR: Author's response | RR: Referee report | ED: Editor decision
ED: Publish subject to revisions (further review by editor and referees) (28 Jan 2020) by Wen Li
AR by Milla Kalliokoski on behalf of the Authors (04 Mar 2020)  Author's response   Manuscript 
ED: Referee Nomination & Report Request started (08 Mar 2020) by Wen Li
RR by Anonymous Referee #1 (09 Mar 2020)
RR by Anonymous Referee #2 (06 Apr 2020)
ED: Publish subject to minor revisions (review by editor) (12 Apr 2020) by Wen Li
AR by Milla Kalliokoski on behalf of the Authors (21 Apr 2020)  Author's response   Manuscript 
ED: Publish as is (27 Apr 2020) by Wen Li
AR by Milla Kalliokoski on behalf of the Authors (27 Apr 2020)
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Short summary
We present a comprehensive statistical study of the response of the Earth's space environment in sheath regions prior to interplanetary coronal mass ejections. The inner magnetospheric wave activity is enhanced in sheath regions, and the sheaths cause significant changes to the outer radiation belt electron fluxes over short timescales. We also show that non-geoeffective sheaths can result in a significant response.