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A comparison of positions and sizes of sources of centimeter and X-ray burstsResults are reported for a parallel study of three centimeter-wave radio bursts observed on August 9, 1973, with the NRAO three-element interferometer at 3.7 and 11.1 cm and the associated X-ray flares observed with the S-054 telescope aboard Skylab. Within the errors of the measurements, the radio and X-ray events are cospatial. Good agreement is found between the size of the X-ray kernel and that of the core of the centimeter burst, but there is evidence that much of the impulsive radio flux was produced in a larger area.
Document ID
19770040950
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Kundu, M. R.
(American Science and Engineering, Inc. Cambridge, MA, United States)
Alissandrakis, C. E.
(Maryland, University College Park, Md., United States)
Kahler, S. W.
(American Science and Engineering, Inc. Cambridge, Mass., United States)
Date Acquired
August 8, 2013
Publication Date
December 1, 1976
Publication Information
Publication: Solar Physics
Volume: 50
Subject Category
Solar Physics
Accession Number
77A23802
Funding Number(s)
CONTRACT_GRANT: NAS8-27758
CONTRACT_GRANT: NSF GA-43297
CONTRACT_GRANT: NGR-21-002-199
Distribution Limits
Public
Copyright
Other

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