A possible explanation of non-steady-state appearances in X-ray spectra of solar flares

Details A possible explanation of non-steady-state appearances in X-ray spectra of solar flares A possible explanation of non-steady-state appearances in X-ray spectra of solar flares

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...77..177k&link_type=abstract

Solar Physics, vol. 77, Apr. 1982, p. 177-181.

Physics

11

Electron Energy, Electron Plasma, Solar Flares, Solar Spectra, Temporal Resolution, X Ray Spectra, Electron Transitions, Forbidden Transitions, Ionization

Scientific paper

Certain peculiarities in solar flare spectra can be qualitatively explained by conceiving of an intense flare as consisting of many short elementary flares (EF) randomly distributed over some space region and time interval. Time-resolved characteristics of such a composed flare can be deduced from time-integrated ones of a single EF if ensemble averaging is replaced by time integration. A comparison of step-rise temperature and essentially transient ionization models is made. Different ions can show discrepancies in electron temperature under the two models.

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