DATA-DRIVEN RADIATIVE HYDRODYNAMIC MODELING OF THE 2014 MARCH 29 X1.0 SOLAR FLARE

ABSTRACT Spectroscopic observations of solar flares provide critical diagnostics of the physical conditions in the flaring atmosphere. Some key features in observed spectra have not yet been accounted for in existing flare models. Here we report a data-driven simulation of the well-observed X1.0 fla...

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Veröffentlicht in:	The Astrophysical journal 2016-08, Vol.827 (1), p.38-38
Hauptverfasser:	Costa, Fatima Rubio da, Kleint, Lucia, Petrosian, Vahé, Liu, Wei, Allred, Joel C.
Format:	Artikel
Sprache:	eng
Schlagworte:	ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Atmospheric models CHROMOSPHERE COMPARATIVE EVALUATIONS Computer simulation ELECTRON DENSITY ELECTRONS EMISSION Flares Fluid flow HARD X RADIATION HYDRODYNAMICS INTERFACES LAYERS line: profiles RADIANT HEAT TRANSFER radiative transfer SIMULATION SOLAR FLARES Solar Physics SPECTRA SUN Sun: chromosphere Sun: flares TELESCOPES VELOCITY
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