Chromospheric emission from nanoflare heating in RADYN simulations
Context. Heating signatures from small-scale magnetic reconnection events in the solar atmosphere have proven to be difficult to detect through observations. Numerical models that reproduce flaring conditions are essential in understanding how nanoflares may act as a heating mechanism of the corona....
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Published in | Astronomy and astrophysics (Berlin) Vol. 659; p. A186 |
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Main Authors | , , , , , , |
Format | Journal Article |
Language | English |
Published |
Heidelberg
EDP Sciences
01.03.2022
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Subjects | |
Online Access | Get full text |
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