The limb flare of 1980 April 30 as seen by the hard X-ray imaging spectrometer

Details The limb flare of 1980 April 30 as seen by the hard X-ray imaging spectrometer The limb flare of 1980 April 30 as seen by the hard X-ray imaging spectrometer

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...244l.157v&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 244, Mar. 15, 1981, p. L157-L162.

Other

29

Solar Flares, Solar Limb, Solar Maximum Mission, Solar X-Rays, X Ray Spectroscopy, High Energy Electrons, Solar Spectrometers, Temperature Distribution, Time Dependence, X Ray Imagery

Scientific paper

X-ray imaging of the limb event of 1980 April 30 shows that the flaring involved two distinct components: a pointlike component, which was the source of the initial hard X-ray burst and an extensive tongue reaching some 30,000 km above the limb. The tongue had a higher temperature than the other parts of the structure and seemed to be enhanced by energetic electrons that derived their energy from the initial source.

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