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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Bibliographic Details
Published inAstronomy and astrophysics (Berlin) Vol. 659; p. A186
Main Authors Bakke, H., Carlsson, M., Rouppe van der Voort, L., Gudiksen, B. V., Polito, V., Testa, P., De Pontieu, B.
Format Journal Article
LanguageEnglish
Published Heidelberg EDP Sciences 01.03.2022
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