Vertical structure of hard X-ray flare

Details Vertical structure of hard X-ray flare Vertical structure of hard X-ray flare

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...86..313t&link_type=abstract

(Japan Society for the Promotion of Science and National Science Foundation, U.S.-Japan Seminar on the Recent Advances in the Un

Physics

34

Coronal Loops, Solar Flares, Solar X-Rays, X Ray Imagery, Chromosphere, H Alpha Line, Solar Electrons

Scientific paper

This paper presents studies of the vertical structure of hard X-ray flares for two contrasting examples. The 1981 May 13 flare contained a coronal hard X-ray source which was located above 50000 km above the photosphere. On the other hand, the 1981 July 20 flare had a chromospheric double source structure in the initial phase. Electrons in this case were able to stream freely from the corona to the chromosphere.

Affiliated with

Also associated with

No associations

Rating

Vertical structure of hard X-ray flare 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 Vertical structure of hard X-ray flare, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Vertical structure of hard X-ray flare will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1628991