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A storm of type 3 bursts observed by RAE-1 in August 1968Curves of the number of type 3 bursts as a function of time are presented for six fixed frequencies (2.8, 1.65, 1.31, 0.995, 0.700, and 0.54 MHz). The curves peak at approximately 0500 UT August 20, 1968, and are symmetrical on both sides. Sakurai (1971) has shown that this time correlates well with the CMP of the McMath Region 9597. The maximum rate of bursts is approximately 150 per hour at the higher frequency of 2.8 MHz. Over 20,000 bursts were counted during the 15-day period from August 13 to August 27 when the active region was visible to the earth. A least-squares normal curve has been fitted to the observational data and calculations of variance and standard deviation are given.
Document ID
19740013368
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Howard, E. G.
(Martin Marietta Corp. Denver, CO, United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1973
Publication Information
Publication: NASA, Washington High Energy Phenomena on the Sun
Subject Category
Space Radiation
Accession Number
74N21481
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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