Statistical Properties of Sub‐Ion Magnetic Holes in the Dipolarized Magnetotail: Formation, Structure, and Dynamics-Reference-Cited by-同舟云学术

Statistical Properties of Sub‐Ion Magnetic Holes in the Dipolarized Magnetotail: Formation, Structure, and Dynamics

Published:2019-01 Issue:1 Volume:124 Page:342-359
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Shustov P. I.¹²^ORCID,Zhang X.‐J.³^ORCID,Pritchett P. L.⁴^ORCID,Artemyev A. V.¹³^ORCID,Angelopoulos V.³,Yushkov E. V.¹²^ORCID,Petrukovich A. A.¹^ORCID

Affiliation:

1. Space Research InstituteRussian Academy of Sciences Moscow Russia

2. Department of PhysicsMoscow State University Moscow Russia

3. Department of Earth, Planetary, and Space SciencesUniversity of California Los Angeles CA USA

4. Department of Physics and AstronomyUniversity of California Los Angeles CA USA

Funder

National Aeronautics and Space Administration

Russian Foundation for Basic Research

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2018JA025852

Reference96 articles.

1. Characteristics of ion flow in the quiet state of the inner plasma sheet

2. First Results from the THEMIS Mission

3. Proton/electron temperature ratio in the magnetotail

4. Adiabatic electron heating in the magnetotail current sheet: Cluster observations and analytical models

5. Electron pitch angle/energy distribution in the magnetotail

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