Ion density and temperature profiles along ( X GSM ) and across ( Z GSM ) the magnetotail as observed by THEMIS, Geotail, and ARTEMIS-Reference-Cited by-同舟云学术

Ion density and temperature profiles along ( X GSM ) and across ( Z GSM ) the magnetotail as observed by THEMIS, Geotail, and ARTEMIS

Published:2017-02 Issue:2 Volume:122 Page:1590-1599
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Artemyev A. V.¹²^ORCID,Angelopoulos V.¹,Hietala H.¹^ORCID,Runov A.¹^ORCID,Shinohara I.³^ORCID

Affiliation:

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

2. Space Research Institute, RAS Moscow Russia

3. Institute of Space and Astronautical ScienceJapan Aerospace Exploration Agency Sagamihara Japan

Funder

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2016JA023710

Reference52 articles.

1. The THEMIS Mission

2. Tail Reconnection Triggering Substorm Onset

3. Kinetic Structure of Current Sheets in the Earth Magnetotail

4. Proton velocity distribution in thin current sheets: Cluster observations and theory of transient trajectories

5. Proton/electron temperature ratio in the magnetotail

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