Scaling of Electron Heating by Magnetization During Reconnection and Applications to Dipolarization Fronts and Super‐Hot Solar Flares-Reference-Cited by-同舟云学术

Scaling of Electron Heating by Magnetization During Reconnection and Applications to Dipolarization Fronts and Super‐Hot Solar Flares

Published:2022-08 Issue:8 Volume:127 Page:
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:JGR Space Physics

Author:

Barbhuiya M. Hasan¹^ORCID,Cassak P. A.¹^ORCID,Shay M. A.²^ORCID,Roytershteyn Vadim³^ORCID,Swisdak M.⁴^ORCID,Caspi Amir⁵^ORCID,Runov Andrei⁶^ORCID,Liang Haoming⁷^ORCID

Affiliation:

1. Department of Physics and Astronomy and the Center for KINETIC Plasma Physics West Virginia University Morgantown WV USA

2. Department of Physics and Astronomy and the Bartol Research Center University of Delaware Newark DE USA

3. Space Science Institute Boulder CO USA

4. Institute for Research in Electronics and Applied Physics University of Maryland College Park MD USA

5. Southwest Research Institute Boulder CO USA

6. Department of Earth and Space Sciences University of California Los Angeles Los Angeles CA USA

7. Center for Space Plasma and Aeronomic Research University of Alabama in Huntsville Huntsville AL USA

Funder

National Science Foundation

National Aeronautics and Space Administration

U.S. Department of Energy

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2022JA030610

Reference98 articles.

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2. Bursty bulk flows in the inner central plasma sheet

3. Tail Reconnection Triggering Substorm Onset

4. Electromagnetic Energy Conversion at Reconnection Fronts

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