Coronal Heating, Weak MHD Turbulence, and Scaling Laws
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference22 articles.
1. Scaling Law for the Heating of Solar Coronal Loops
2. Magnetohydrodynamic Turbulence of Coronal Active Regions and the Distribution of Nanoflares
3. Energy spectrum of turbulent fluctuations in boundary driven reduced magnetohydrodynamics
4. The distribution of flares, statistics of magnetohydrodynamic turbulence and coronal heating
5. Energy Release in a Turbulent Corona
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1. Steadiness of Coronal Heating;The Astrophysical Journal;2023-10-23
2. Fast magneto-acoustic wave turbulence and the Iroshnikov–Kraichnan spectrum;Journal of Plasma Physics;2023-03-31
3. Alfvénic waves in the inhomogeneous solar atmosphere;Reviews of Modern Plasma Physics;2023-03-21
4. Solar Coronal Heating Fueled by Random Bursts of Fine-scale Magnetic Reconnection in Turbulent Plasma Regions;The Astrophysical Journal;2023-02-01
5. Do chaotic field lines cause fast reconnection in coronal loops?;Physics of Plasmas;2022-12
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