EXPLOSIVE INSTABILITY AND CORONAL HEATING
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference31 articles.
1. Instability Mechanisms in Shear-Flow Transition
2. Transition to turbulent electric current sheet reconnection
3. Secondary instability in three‐dimensional magnetic reconnection
4. Coronal energy release via ideal three-dimensional instability three-dimensional instability
5. An Explanation for the “Switch‐On” Nature of Magnetic Energy Release and Its Application to Coronal Heating
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1. The Location and Angle Distribution of Magnetic Reconnection in the Solar Corona;The Astrophysical Journal;2022-10-01
2. Synchronization of Small-scale Magnetic Features, Blinkers, and Coronal Bright Points;The Astrophysical Journal;2022-02-01
3. The Heating of the Solar Corona;Solar Physics and Solar Wind;2021-04-12
4. Plasma physics and astrophysics: retrospects, state-of-the art, and prospects;Rendiconti Lincei. Scienze Fisiche e Naturali;2020-11-23
5. The Onset of 3D Magnetic Reconnection and Heating in the Solar Corona;The Astrophysical Journal;2020-03-04
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