The solar flare of 1980 July 14 and the emergent magnetic flux model

Details The solar flare of 1980 July 14 and the emergent magnetic flux model The solar flare of 1980 July 14 and the emergent magnetic flux model

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984cha%26a...8...89t&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 8, Issue 1, p. 89-93.

Astronomy and Astrophysics

Astrophysics

Scientific paper

We make a combined study of the class 3B flare of 1980 July 14 using the Hα patrol, white-light photographs, velocity field measurements of the Yunnan Observatory, the SMM data on X-rays, and the radio observations by the Beijing Observatory. The morphological changes are analysed in terms of the EMF model and a number of physical parameters evaluated. Our results show: 1) that the EMF model is in basic agreement with the observations, 2) that the current sheet could be located at or near the points where the zero velocity line cuts the dark filament and the magnetic neutral line and 3) that the hard tX-ray burst was produced by the non-thermal electrons in the current sheet, while the soft X-ray burst was produced by the thermal bremsstrahlung of a hot plasma in the active region.

Affiliated with

Also associated with

No associations

Rating

The solar flare of 1980 July 14 and the emergent magnetic flux model 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 The solar flare of 1980 July 14 and the emergent magnetic flux model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The solar flare of 1980 July 14 and the emergent magnetic flux model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1040879