Can the Superposition of Evaporative Flows Explain Broad Fe xxi Profiles during Solar Flares?
Author:
Funder
NASA
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/2041-8213/ab290b/pdf
Reference50 articles.
1. A UNIFIED COMPUTATIONAL MODEL FOR SOLAR AND STELLAR FLARES
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3. On magnetic field stochasticity and nonthermal line broadening in solar flares
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5. On the consequences of a non-equilibrium ionisation balance for compact flare emission and dynamics
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