Studies on solar prominences in relation to H-alpha and X-ray flares.

Details Studies on solar prominences in relation to H-alpha and X-ray flares. Studies on solar prominences in relation to H-alpha and X-ray flares.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996injpb..70...81c&link_type=abstract

Indian J. Phys., Part B, Vol. 70B, No. 1, p. 81 - 85

Mathematics

Probability

Solar Prominences: H Alpha, Solar Prominences: Solar X-Ray Flares

Scientific paper

A study has been made of solar prominences in relation to H-alpha flares accompanied by high speed dark filaments (H-type of flares) as well as with X-rays. Most of the H-type flares have areas of 0 - 80 millionths of a solar hemisphere, a rise time of 0 - 5 min and a duration of 0 - 25 min. The time of onset of this kind of flares always precedes that of filaments in most of cases. The H-type flares have a general tendency to be correlated with X-ray flares. But when the probability of their occurrences with respect to all the types of flares was calculated for the frequency distributions of area as well as duration, such probability has been found to increase with the increase of the respective quantities.

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