A magnetohydrodynamic approach for interpreting solar polarization bursts at 7 GHz

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dc.contributor.authorMatsuura O.T.
dc.date.accessioned2024-03-13T01:48:31Z
dc.date.available2024-03-13T01:48:31Z
dc.date.issued1969
dc.description.abstractA magnetohydrodynamic (MHD) approach is presented that appears to be comprehensive for the interpretation of the recently discovered microwave solar events, in which only the degree of circular polarization changes, without any increase in the output of the total solar flux. On the basis of this explanation experimental evidence is suggested for Alfvén waves, in relation to the velocity fields in the solar chromosphere. © 1969 D. Reidel Publishing Company.
dc.description.firstpage173
dc.description.issuenumber1
dc.description.lastpage182
dc.description.volume9
dc.identifier.doi10.1007/BF00145738
dc.identifier.issn0038-0938
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/38122
dc.relation.ispartofSolar Physics
dc.rightsAcesso Restrito
dc.titleA magnetohydrodynamic approach for interpreting solar polarization bursts at 7 GHz
dc.typeArtigo
local.scopus.citations0
local.scopus.eid2-s2.0-34250499139
local.scopus.updated2024-05-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=34250499139&origin=inward
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