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Correlated observations of impulsive UV and hard X-ray bursts in solar flares from the Solar Maximum Mission

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/161854· OSTI ID:6747195
We have studied the temporal and spatial structures of UV and hard X-ray bursts in a disk ad a limb flare observed with instruments on the Solar Maximum Mission. The UV observations were spatially resolved with a resolution of 3''--4'' and were done in the Si IV, O IV lines and in the UV continuum region. The results are: (1) There was considerable preflare activity with UV transient brightenings occurring in many small point-like kernels. The flare later occurred in these active kernels; some of the active kernels, however, did not flare. (2) The impulsie UV and hard X-ray bursts were temporally correlated. Indivudual peaks in the hard X-ray bursts can be identified with individual peaks in the UV bursts of individual flaring kernels. In between the individual maxima, however, the UV emission remained intense. (3) There were impulsie brightenings in the UV continuum during the time of the hard X-ray bursts. (4) For the disk flare, the many flaring kernels were confined in a small area while for the limb flare, the impulsive bursts occurred in two points separated by a large distance of 50'' on the limb. (5)= The UV bursts started to rise earlier than the correspondig hard X-ray bursts. (6) There is some indication that the UV intensity of the bright points actually dropped just before it began to flare and to rise sharply. These results indicate that the emission source of the hard X-ray burst was located in the lower atmosphere where the density is high, and that there was local heating.
Research Organization:
E. O. Hulbert Center for Space Research, Naval Research Laboratory
OSTI ID:
6747195
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 278:2; ISSN ASJOA
Country of Publication:
United States
Language:
English