Energy Flow in the Region 2 Field‐Aligned Current Region Under Quasi‐steady Convection
Author:
Affiliation:
1. Research Institute for Sustainable Humanosphere Kyoto University Uji Japan
2. Institute of Earth Sciences, Academia Sinica Taipei Taiwan
3. ICSWSE Fukuoka Japan
Funder
Ministry of Science and Technology, Taiwan
Japan Society for the Promotion of Science
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Geophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1029/2019JA026998
Reference37 articles.
1. A proposed production model of rapid subauroral ion drifts and their relationship to substorm evolution
2. Postmidnight storm-time enhancement of tens-of-keV proton flux
3. Dynamical property of storm time subauroral rapid flows as a manifestation of complex structures of the plasma pressure in the inner magnetosphere
4. Energy Flow Exciting Field-Aligned Current at Substorm Expansion Onset
5. New Diagnosis for Energy Flow From Solar Wind to Ionosphere During Substorm: Global MHD Simulation
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