Determination of Flare Heating and Cooling Using the [ITAL]Transition Region and Coronal Explorer[/ITAL]
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference9 articles.
1. Evaporative cooling of flare plasma
2. Explosive evaporation in solar flares
3. The formation of flare loops by magnetic reconnection and chromospheric ablation
4. A new view of the solar corona from the transition region and coronal explorer (TRACE)
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1. The Transition Region of Solar Flare Loops;The Astrophysical Journal;2023-02-01
2. The Effect of Thermal Nonequilibrium on Helmet Streamers;The Astrophysical Journal;2021-08-01
3. Multi-wavelength Analysis to Solar Corona Heating Events;Chinese Astronomy and Astrophysics;2015-01
4. Fine structure of the sources of quasi-periodic pulsations in “single-loop” solar flares;Astronomy Letters;2013-04
5. ESTIMATES OF DENSITIES AND FILLING FACTORS FROM A COOLING TIME ANALYSIS OF SOLAR MICROFLARES OBSERVED WITHRHESSI;The Astrophysical Journal;2011-07-06
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