Solar wind‐driven variations of electron plasma sheet densities and temperatures beyond geostationary orbit during storm times-Reference-Cited by-同舟云学术

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Solar wind‐driven variations of electron plasma sheet densities and temperatures beyond geostationary orbit during storm times

Published:2016-09 Issue:9 Volume:121 Page:8343-8360
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Dubyagin S.¹,Ganushkina N. Yu.¹²,Sillanpää I.¹,Runov A.³

Affiliation:

1. Finnish Meteorological Institute Helsinki Finland

2. Climate and Space Sciences and Engineering DepartmentUniversity of Michigan Ann Arbor Michigan USA

3. Institute of Geophysics and Planetary PhysicsUniversity of California Los Angeles California USA

Funder

European Union Seventh Framework Programme

European Union Horizon 2020 Research and Innovation programme

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2016JA022947

Reference49 articles.

1. Proton/electron temperature ratio in the magnetotail

2. Profiles of electron temperature and <I>B</I><sub>z</sub> along Earth's magnetotail

3. The THEMIS Fluxgate Magnetometer

4. Bursty bulk flows in the inner central plasma sheet

5. The THEMIS Mission

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