An analysis of the solar loop flare of March 27, 1979

Details An analysis of the solar loop flare of March 27, 1979 An analysis of the solar loop flare of March 27, 1979

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981scisn..24..656s&link_type=abstract

Scientia Sinica, vol. 24, May 1981, p. 656-661.

Mathematics

Logic

Magnetic Field Configurations, Magnetohydrodynamic Stability, Solar Flares, Solar Limb, Extreme Ultraviolet Radiation, H Alpha Line, Solar Magnetic Field, Solar X-Rays

Scientific paper

A loop flare occurring on March 27, 1979, close to the solar western limb and the morphological features of a pair of rarely-found H-alpha bright kernels in the flare are described in this paper. The relations between the H-alpha bright kernels and MHD instability are discussed briefly. This might, as it seems, provide observational evidence for the sausage-type instability of solar flare.

Affiliated with

Also associated with

No associations

Rating

An analysis of the solar loop flare of March 27, 1979 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 An analysis of the solar loop flare of March 27, 1979, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An analysis of the solar loop flare of March 27, 1979 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1443044