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- W120983635 abstract "We analyze thirteen X-ray line spectra (7.8-23.0 A) acquired during a solar flare that peaked at 2326 UT on 1979 March 31. The data include fluxes of lines excited throughout the temperature range 2-18 million K), the entire range present in the coronal flare. The coronal flare emission measure began to decrease 500 s or less after the broad band X-ray flux peaked. We construct the differential emission measure epsilon(T) for 2-18 million K from the data by using collision strengths now available for a small number of the observed lines. The total emission measure for T greater than 2 million K, the radiative energy loss rate, the density at 2 million K, and the conductive cooling time are derived from the data, but lack of information on electron densities prevents a detailed study of the flare energetics. This situation is unlikely to improve in the near future. Conductive cooling was more important than radiative cooling for coronal temperatures in this flare." @default.
- W120983635 created "2016-06-24" @default.
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- W120983635 date "1981-05-01" @default.
- W120983635 modified "2023-09-27" @default.
- W120983635 title "Analysis of a series of solar flare x-ray spectra. Technical report" @default.
- W120983635 hasPublicationYear "1981" @default.
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