Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...287..917a&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 287, Dec. 15, 1984, p. 917-925. Research supported by the Consiglio Naziona
Astronomy and Astrophysics
Astrophysics
151
Chromosphere, Evaporation, Plasma Turbulence, Solar Flares, Solar Maximum Mission, Solar X-Rays, Bremsstrahlung, Energy Dissipation, Energy Transfer, High Resolution, Mass Transfer, Plasma Diagnostics, Solar Activity Effects, X Ray Spectroscopy
Scientific paper
The Solar Maximum Mission (SMM) spacecraft has provided high time resolution observational data regarding the soft X-ray emission from solar-flare plasma during 1980. The present investigation is concerned with the characteristics of a soft X-ray flare and the energetics of the impulsive phase on the basis of the data collected with the aid of two of the instruments on board the SMM, taking into account the Hard X-ray Burst Spectrometer (HXRBS) and the Bent Crystal Spectrometer (BCS). Attention is given to an analysis of soft X-ray flare spectra, the relative motion of the soft X-ray sources, the phenomenology of the soft X-ray flare, energy and mass transport during the impulsive phase, and energy deposition in the chromosphere during evaporation.
Antonucci Ester
Dennis Brian R.
Gabriel Alan H.
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