An impulsive solar burst observed in H-alpha, microwaves, and hard X-rays

Details An impulsive solar burst observed in H-alpha, microwaves, and hard X-rays An impulsive solar burst observed in H-alpha, microwaves, and hard X-rays

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...288..385g&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 288, Jan. 1, 1985, p. 385-395.

Astronomy and Astrophysics

Astrophysics

11

H Alpha Line, Microwave Emission, Solar Flares, Solar Radio Bursts, Solar X-Rays, Electron Acceleration, Electron Energy, Interferometry, Least Squares Method, X Ray Spectroscopy

Scientific paper

The authors present Hα, 10.6 GHz microwave, and greater than 100 keV X-ray observations of a single impulsive spike flare that occurred on 1980 May 28, 1947 UT. The isolated high flux spike provides an excellent opportunity to infer the time behavior of the electron acceleration that is assumed to yield the microwave and hard X-ray flux profiles. It is found that, although the time profile consists of a simple, single peak, the spike is actually due to two acceleration episodes in separate sources. The authors adopt a source model for microwave and hard X-ray sources, in which the microwave source is due to electrons trapped at the top of a magnetic loop, and the hard X-ray source is due to thick-target emission at the footpoints.

Affiliated with

Also associated with

No associations

Rating

An impulsive solar burst observed in H-alpha, microwaves, and hard X-rays 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 impulsive solar burst observed in H-alpha, microwaves, and hard X-rays, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An impulsive solar burst observed in H-alpha, microwaves, and hard X-rays will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-925299