Polarization bursts in the sun observed at microwave frequencies

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dc.contributor.authorKaufmann P.
dc.contributor.authorMatsuura O.T.
dc.contributor.authorMascaro A.C.M.
dc.contributor.authorMendes A.M.
dc.date.accessioned2024-05-08T14:04:39Z
dc.date.available2024-05-08T14:04:39Z
dc.date.issued1968
dc.description.abstractThere are microwave bursts not observable in the total flux from the Sun, but only in circular polarization. The production of these events in the Sun requires equivalent changes of the magnetic field imposed on the emission regions during the bursts. © 1968 Nature Publishing Group.
dc.description.firstpage1298
dc.description.issuenumber5174
dc.description.lastpage1300
dc.description.volume220
dc.identifier.doi10.1038/2201298a0
dc.identifier.issn0028-0836
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/38699
dc.relation.ispartofNature
dc.rightsAcesso Restrito
dc.titlePolarization bursts in the sun observed at microwave frequencies
dc.typeArtigo
local.scopus.citations3
local.scopus.eid2-s2.0-36949053984
local.scopus.updated2024-03-12
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=36949053984&origin=inward
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