Analysis of the X-ray/Hα flare of 1980 July 14

Details Analysis of the X-ray/Hα flare of 1980 July 14 Analysis of the X-ray/Hα flare of 1980 July 14

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985cha%26a...9..164x&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 9, Issue 2, p. 164-169.

Astronomy and Astrophysics

Astrophysics

Scientific paper

Using the X-ray data from the SMM Satellite and the optical data from the Yunnan Observatory, we analysed the Class 3B flare of 1980 July 14. We obtained the time variation of the X-ray spectrum, calculated the total number of electrons at the time of the flare and their mean energy and measured and compared the positions of the Hα flare and the X-ray burst source. The results show 1) that the hard X-ray burst was caused by high-energy non-thermal electron beam; 2) that the soft X-ray burst was basically generated by thermal bremsstrahlung of hot plasma, but the contribution by non-thermal electrons must also be included; 3) that the determined height of the X-ray burst source depends on the flare model and the magnetic field configuration of the active region. The results obtained support the newly emergent flux model of flares.

Affiliated with

Also associated with

No associations

Rating

Analysis of the X-ray/Hα flare of 1980 July 14 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 Analysis of the X-ray/Hα flare of 1980 July 14, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Analysis of the X-ray/Hα flare of 1980 July 14 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1666838