Solar micro-bursts at 22.2 GHz and their relationship to events observed at lower frequencies

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dc.contributor.authorBlakey J.R.
dc.date.accessioned2024-03-13T01:47:56Z
dc.date.available2024-03-13T01:47:56Z
dc.date.issued1976
dc.description.abstractObservations of McMath region 10433 at 22 GHz using a telescope with a 4′ beam during July 1974 revealed the existence events or 'microbursts' with intensities below the sensitivity limit of normal solar patrol instruments. Many of these events were simply the high frequency counterpart of more intense bursts observed at lower frequencies. This note considers the small number of events which suggest that the gyro-synchrotron mechanism alone is incapable of explaining the observations and indicates that a thermal mechanism is needed to explain the high frequency event. © 1976 D. Reidel Publishing Company.
dc.description.firstpage241
dc.description.issuenumber1
dc.description.lastpage245
dc.description.volume46
dc.identifier.doi10.1007/BF00157570
dc.identifier.issn0038-0938
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/38089
dc.relation.ispartofSolar Physics
dc.rightsAcesso Restrito
dc.titleSolar micro-bursts at 22.2 GHz and their relationship to events observed at lower frequencies
dc.typeArtigo
local.scopus.citations3
local.scopus.eid2-s2.0-34250381663
local.scopus.updated2024-05-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=34250381663&origin=inward
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