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Correlated observations of a spatially resolved type III solar radio burst group and the associated hard X-ray emissionThe first measurements of the spatial structure of a group of type III solar radio bursts associated with an impulsive hard X-ray burst are presented. At 169 MHz the radio source has been found to consist of two principal regions separated by about 300,000 km. The two regions together produced a total of four component bursts in good time correlation with spikes in the hard X-ray emission. The observations indicate that electron acceleration/injection occurs over a region which covers a wide range of magnetic field lines.
Document ID
19810031693
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Kane, S. R.
(Observatoire de Paris-Meudon France)
Pick, M.
(Observatoire de Paris-Meudon France)
Raoult, A.
(Paris, Observatoire, Meudon Hauts-de-Seine, France)
Date Acquired
August 11, 2013
Publication Date
October 15, 1980
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Accession Number
81A16097
Funding Number(s)
CONTRACT_GRANT: NAS5-22307
Distribution Limits
Public
Copyright
Other

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