Strong Photospheric Heating Indicated by Fe i 6173 Å Line Emission during White-light Solar Flares

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Strong Photospheric Heating Indicated by Fe i 6173 Å Line Emission during White-light Solar Flares

Between 2017 and 2024, the Helioseismic and Magnetic Imager (HMI) on board the Solar Dynamics Observatory has observed numerous white-light solar flares (WLFs). HMI spectropolarimetric observations of certain WLFs, in particular the X9.3 flare of 2017 September 6, reveal one or more locations within...

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Bibliographic Details
Main Authors:	Samuel Granovsky, Alexander G. Kosovichev, Viacheslav M. Sadykov, Graham S. Kerr, Joel C. Allred
Format:	Article
Language:	English
Published:	IOP Publishing 2025-01-01
Series:	The Astrophysical Journal
Subjects:	Solar flares
Online Access:	https://doi.org/10.3847/1538-4357/addd1e
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