Plasma Pressure Profiles in the Dark Sector of the Earth’s Magnetosphere during the Magnetic Storm of May 29, 2010
- Authors: Kirpichev I.P.1, Antonova E.E.2,1
-
Affiliations:
- Space Research Institute, Russian Academy of Sciences
- Scobeltsyn Institute of Nuclear Physics, Moscow State University
- Issue: Vol 58, No 6 (2018)
- Pages: 710-717
- Section: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/156938
- DOI: https://doi.org/10.1134/S0016793218060075
- ID: 156938
Cite item
Abstract
Variations in the radial profile of the pressure and distortions of the magnetic field of the magnetosphere in the dark sector near the equatorial plane during the storm of May 29, 2010, are analyzed based on THEMIS data. The position of the pressure maximum during the main phase of the storm is determined. The time dynamics of the pressure maximum is traced during the recovery phase. The time of pressure relaxation to initial values (before the main phase) during the recovery phase are assessed. The coincidence of the positions of the pressure peak maximum and of maximal deviation of the magnetic field from the dipole one is ascertained.
About the authors
I. P. Kirpichev
Space Research Institute, Russian Academy of Sciences
Author for correspondence.
Email: ikir@iki.rssi.ru
Russian Federation, Moscow
E. E. Antonova
Scobeltsyn Institute of Nuclear Physics, Moscow State University; Space Research Institute, Russian Academy of Sciences
Author for correspondence.
Email: elizaveta.antonova@gmail.com
Russian Federation, Moscow; Moscow
Supplementary files
