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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Latest update: 06 Oct 2025
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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.
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