Response of SDO/HMI Observables to Heating of the Solar Atmosphere by Precipitating High-energy Electrons

We perform an analysis of the line-of-sight (LOS) observables of the Helioseismic and Magnetic Imager (HMI) on board the Solar Dynamics Observatory (SDO) for models of the solar atmosphere heated by precipitating high-energy electrons during solar flares. The radiative hydrodynamic (RADYN) flare mod...

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Veröffentlicht in:	The Astrophysical journal 2020-04, Vol.893 (1), p.24
Hauptverfasser:	Sadykov, Viacheslav M., Kosovichev, Alexander G., Kitiashvili, Irina N., Kerr, Graham S.
Format:	Artikel
Sprache:	eng
Schlagworte:	Algorithms Astrophysics Atmosphere Atmospheric models Data processing Energy flux Heating High energy electrons Line of sight Magnetic fields Magnetism Radiative transfer Solar activity Solar atmosphere Solar energy Solar flares Solar magnetic fields Solar observatories Solar photosphere Spectropolarimetry
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