A statistical analysis of hard X-Ray solar flares

Details A statistical analysis of hard X-Ray solar flares A statistical analysis of hard X-Ray solar flares

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.208...99p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 208, no. 1, p. 99-111

Astronomy and Astrophysics

Astrophysics

31

Solar Flares, Solar X-Rays, Statistical Analysis, Asymmetry, Flux (Rate), Flux Density, Solar Maximum Mission, Spectral Energy Distribution, Time

Scientific paper

In this study we perform a statistical study on, 8319 X-Ray solar flares observed with the Hard X-Ray Spectrometer (HXRBS) on the Solar Maximum Mission satellite (SMM). The events are examined in terms of the durations, maximum intensities, and intensity profiles. It is concluded that there is no evidence for a correlation between flare intensity, flare duration, and flare asymmetry. However, we do find evidence for a rapid fall-of in the number of short-duration events.

Affiliated with

Also associated with

No associations

Rating

A statistical analysis of hard X-Ray solar flares does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A statistical analysis of hard X-Ray solar flares, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A statistical analysis of hard X-Ray solar flares will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1324007