The Occurrence Probability of X-rays Plasma Ejections by Solar Flares

Details The Occurrence Probability of X-rays Plasma Ejections by Solar Flares The Occurrence Probability of X-rays Plasma Ejections by Solar Flares

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aspc..205..137a&link_type=abstract

Last Total Solar Eclipse of the Millennium, ASP Conference Series, Vol. 205. Edited by W. Livingston and A. Özgüç. ISBN: 1-58

Mathematics

Probability

2

Scientific paper

We have investigated X-ray ejecta above flare loops, which were observed before soft X-ray peak time, using the Yohkoh soft X-ray observations in 1996 when the background corona was very weak. We found 35 plasma ejecta out of 84 flares and studied soft X-ray data to discover the probability to observe the plasma ejecta. On the other hand, we searched for prominence eruptions using Solar-Geophysical Data in the same flare series and found 16 prominence eruptions out of 29 flares having soft x-ray plasma ejecta. As a result, 76% of flares have plasma ejecta observed in either Hα or soft X-ray wavelength. It follows from this that there are many flare associated ejecta.

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