Thin Current Sheet Formation and Reconnection at X ∼ −10 R E During the Main Phase of a Magnetic Storm-Reference-Cited by-同舟云学术

Thin Current Sheet Formation and Reconnection at X ∼ −10 R _E During the Main Phase of a Magnetic Storm

Published:2022-09 Issue:9 Volume:127 Page:
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:JGR Space Physics

Author:

Runov A.¹^ORCID,Angelopoulos V.¹^ORCID,Weygand J. M.¹^ORCID,Artemyev A. V.¹^ORCID,Beyene F.¹^ORCID,Sergeev V.²^ORCID,Kubyshkina M.²^ORCID,Henderson M. G.³^ORCID

Affiliation:

1. Department of Earth, Planetary, and Space Sciences Institute of Geophysics and Planetary Physics University of California Los Angeles CA USA

2. St. Petersburg University St.Petersburg Russia

3. Los Alamos National Laboratory Los Alamos NM USA

Funder

National Aeronautics and Space Administration

Ministry of Education and Science of the Russian Federation

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2022JA030669

Reference57 articles.

1. Ionospheric disturbance magnetic field continuation from the ground to the ionosphere using spherical elementary current systems

2. The ARTEMIS Mission

3. Near-Earth magnetotail reconnection powers space storms

4. First Results from the THEMIS Mission

5. Correcting the NOAA/MEPED energetic electron fluxes for detector efficiency and proton contamination

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