A Solar Magnetic-fan Flaring Arch Heated by Nonthermal Particles and Hot Plasma from an X-Ray Jet Eruption
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab8bce/pdf
Reference126 articles.
1. Electron Time-of-Flight Distances and Flare Loop Geometries Compared from CGRO and YOHKOH Observations
2. Hard X-ray emission from a flare-related jet
3. SUPPRESSION OF PARALLEL TRANSPORT IN TURBULENT MAGNETIZED PLASMAS AND ITS IMPACT ON THE NON-THERMAL AND THERMAL ASPECTS OF SOLAR FLARES
4. THE COOLING OF CORONAL PLASMAS. III. ENTHALPY TRANSFER AS A MECHANISM FOR ENERGY LOSS
5. Coronal Loop Scaling Laws for Various Forms of Parallel Heat Conduction
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3. Imaging and Spectroscopic Observations of the Dynamic Processes in Limb Solar Flares;The Astrophysical Journal;2022-08-01
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