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Observations of H. cap alpha. and microwave brightening caused by a distant solar flare

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/160750· OSTI ID:6268978
Three subflares were observed at 6 cm lambda and at H ..cap alpha.. (6563 A) with the NRAO Very Large Array (VLA) and the Solar Observing Optical Network (SOON) high resolution telescopes. Synthesized maps with integration times of 10 and 30 s show that most of the 6 cm burst emission originated in approx. 10''-15'' features coincident with or adjacent to H ..cap alpha.. flare kernels. The brightness temperatures of the radio features ranged from 3 x 10/sup 7/ to 9 x 10/sup 7/ K. During the onset of one of the subflares 6 cm emission was discovered in a loop stretching>10/sup 5/ km from the pirmary flare site; this emission was associated with faint H..cap alpha.. flarelike brightness at the remote footpoint of the loop. Assuming that the energy for the distant brightening originated at the primary flare site, we find that approx.4 x 10/sup 24/ ergs s/sup -1/ propagated along the connecting magnetic loop at a velocity of > or =6000 km s/sup -1/. We discuss various possible mechanisms for the distant activation. We rule out MHD shocks and thermal conduction fronts as the exciting agents. We suggest that the energy may have been carried by electrons originating in the high energy tail of the electron thermal velocity distribution and escaping from the primary flare site.
Research Organization:
Astronomy Program, University of Maryland
OSTI ID:
6268978
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 265:2; ISSN ASJOA
Country of Publication:
United States
Language:
English