Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph..102..111b&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 102, no. 1-2, Dec. 1985, p. 111-130. Research supported by the Lockheed Independent Researc
Astronomy and Astrophysics
Astronomy
2
Light Curve, Plasma Diagnostics, Plasma Temperature, Solar Flares, X Ray Astronomy, Decay, Flux Quantization, Plasma Radiation, Solar Maximum Mission
Scientific paper
The light curves of soft X-ray lines, observed by the Flat Crystal Spectrometer on Solar Maximum Mission during eight solar flares are modeled to determine the plasma temperature and emission measure as functions of time using the method first presented by Bornmann (1985), but modified to include a χ2search routine. With this modification the technique becomes more general, more accurate, and applicable throughout the gradual phase of the flare. The model reproduces the light curves of the soft X-ray lines throughout these flares. Model fits were repeated for each flare using five different sets of published line emissivity calculations. The emissivities of Mewe and Gronenschild (1981) consistently gave the best fits to the observed light curves for each flare.
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