Characteristics of the Flank Magnetopause: THEMIS Observations.
Journal
Journal of geophysical research. Space physics
ISSN: 2169-9380
Titre abrégé: J Geophys Res Space Phys
Pays: United States
ID NLM: 101661799
Informations de publication
Date de publication:
May 2019
May 2019
Historique:
received:
01
01
2019
revised:
01
04
2019
accepted:
30
04
2019
entrez:
20
8
2019
pubmed:
20
8
2019
medline:
20
8
2019
Statut:
ppublish
Résumé
The terrestrial magnetopause is the boundary that shields the Earth's magnetosphere on one side from the shocked solar wind and its embedded interplanetary magnetic field on the other side. In this paper, we show observations from two of the Time History of Events and Macroscales Interactions during Substorms (THEMIS) satellites, comparing dayside magnetopause crossings with flank crossings near the terminator. Macroscopic properties such as current sheet thickness, motion, and current density are examined for a large number of magnetopause crossings. The results show that the flank magnetopause is typically thicker than the dayside magnetopause and has a lower current density. Consistent with earlier results from Cluster observations, we also find a persistent dawn-dusk asymmetry with a thicker and more dynamic magnetopause at dawn than at dusk.
Identifiants
pubmed: 31423410
doi: 10.1029/2019JA026459
pii: JGRA54959
pmc: PMC6686701
doi:
Types de publication
Journal Article
Langues
eng
Pagination
3421-3435Références
Nat Commun. 2015 May 11;6:7019
pubmed: 25960122
J Geophys Res Space Phys. 2019 May;124(5):3421-3435
pubmed: 31423410