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Characteristics of the Flank Magnetopause: THEMIS Observations

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 d...

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Detalles Bibliográficos
Autores principales: Haaland, S., Runov, A., Artemyev, A., Angelopoulos, V.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: John Wiley and Sons Inc. 2019
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6686701/
https://www.ncbi.nlm.nih.gov/pubmed/31423410
http://dx.doi.org/10.1029/2019JA026459
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author Haaland, S.
Runov, A.
Artemyev, A.
Angelopoulos, V.
author_facet Haaland, S.
Runov, A.
Artemyev, A.
Angelopoulos, V.
author_sort Haaland, S.
collection PubMed
description 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.
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spelling pubmed-66867012019-08-14 Characteristics of the Flank Magnetopause: THEMIS Observations Haaland, S. Runov, A. Artemyev, A. Angelopoulos, V. J Geophys Res Space Phys Research Articles 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. John Wiley and Sons Inc. 2019-05-30 2019-05 /pmc/articles/PMC6686701/ /pubmed/31423410 http://dx.doi.org/10.1029/2019JA026459 Text en ©2019. The Authors. This is an open access article under the terms of the http://creativecommons.org/licenses/by-nc-nd/4.0/ License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non‐commercial and no modifications or adaptations are made.
spellingShingle Research Articles
Haaland, S.
Runov, A.
Artemyev, A.
Angelopoulos, V.
Characteristics of the Flank Magnetopause: THEMIS Observations
title Characteristics of the Flank Magnetopause: THEMIS Observations
title_full Characteristics of the Flank Magnetopause: THEMIS Observations
title_fullStr Characteristics of the Flank Magnetopause: THEMIS Observations
title_full_unstemmed Characteristics of the Flank Magnetopause: THEMIS Observations
title_short Characteristics of the Flank Magnetopause: THEMIS Observations
title_sort characteristics of the flank magnetopause: themis observations
topic Research Articles
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6686701/
https://www.ncbi.nlm.nih.gov/pubmed/31423410
http://dx.doi.org/10.1029/2019JA026459
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