Your browser doesn't support javascript.
loading
Characteristics of the Flank Magnetopause: THEMIS Observations.
Haaland, S; Runov, A; Artemyev, A; Angelopoulos, V.
Afiliación
  • Haaland S; Birkeland Centre for Space Science University of Bergen Bergen Norway.
  • Runov A; Max-Planck Institute for Solar Systems Research Göttingen Germany.
  • Artemyev A; Department of Space Physics University of California Los Angeles CA USA.
  • Angelopoulos V; Department of Space Physics University of California Los Angeles CA USA.
J Geophys Res Space Phys ; 124(5): 3421-3435, 2019 May.
Article en En | MEDLINE | ID: mdl-31423410
ABSTRACT
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.

Texto completo: 1 Colección: 01-internacional Base de datos: MEDLINE Idioma: En Revista: J Geophys Res Space Phys Año: 2019 Tipo del documento: Article

Texto completo: 1 Colección: 01-internacional Base de datos: MEDLINE Idioma: En Revista: J Geophys Res Space Phys Año: 2019 Tipo del documento: Article