Polarization of a periodic solar microwave burst

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dc.contributor.authorKaufmann P.
dc.date.accessioned2024-03-13T01:47:55Z
dc.date.available2024-03-13T01:47:55Z
dc.date.issued1976
dc.description.abstractNo fluctuations in polarization have been found during a 7 GHz solar burst showing 17 s periodic pulses in intensity. Polarization effects can be produced by the propagation media in the active centre, which are not affected directly by the burst source, but situated more deeply than the observed heights at that microwave frequency. © 1976 D. Reidel Publishing Company.
dc.description.firstpage197
dc.description.issuenumber1
dc.description.lastpage199
dc.description.volume50
dc.identifier.doi10.1007/BF00206201
dc.identifier.issn0038-0938
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/38088
dc.relation.ispartofSolar Physics
dc.rightsAcesso Restrito
dc.titlePolarization of a periodic solar microwave burst
dc.typeArtigo
local.scopus.citations2
local.scopus.eid2-s2.0-34250385369
local.scopus.updated2024-05-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=34250385369&origin=inward
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