The thermal phase of a large solar flare

EUV and X-ray observations are used to derive the differential emission measures, temperatures, densities, radiative and conductive cooling rates, and thermal energy content of a class 2B flare that occurred on 1973 September 7. The results of the analysis indicate that (1) most of the flare plasma...

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Bibliographische Detailangaben
Veröffentlicht in:	Astrophys. J.; (United States) 1978-10, Vol.225, p.641
1. Verfasser:	Withbroe, G. L.
Format:	Artikel
Sprache:	eng
Schlagworte:	CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS COOLING ELECTROMAGNETIC RADIATION ENERGY TRANSFER FAR ULTRAVIOLET RADIATION HEAT TRANSFER IONIZING RADIATIONS MATHEMATICAL MODELS PLASMA RADIATIONS RADIATIVE COOLING SOLAR ACTIVITY SOLAR FLARES STAR MODELS THERMAL CONDUCTION ULTRAVIOLET RADIATION 640104 > Astrophysics & Cosmology-- Solar Phenomena X RADIATION
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