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Structure of proton centers and associated nonthermal bursts at microwave frequenciesA very broad band of electromagnetic radiation is emitted during solar flares, especially at the explosive phase. The existence of a large variety of plasmas with various densities and a wide range of temperatures or energies is proposed as the initiating agent. The manner in which the plasmas are heated and accelerated to subrelativistic and relativistic energies is discussed. Observational evidence on the characteristics of active regions which produced proton flares and on the structure of the associated nonthermal microwave bursts of the sun is presented. The behavior of subrelativistic electrons on the sun is described.
Document ID
19740013333
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Enome, S.
(Nagoya Univ. Aichi, Japan)
Tanaka, H.
(Nagoya Univ. Aichi, Japan)
Date Acquired
August 7, 2013
Publication Date
January 1, 1973
Publication Information
Publication: NASA, Washington High Energy Phenomena on the Sun
Subject Category
Communications
Accession Number
74N21446
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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