On the long-term behaviour of the circular polarization from coronal condensation radio emission at 4.3 cm wavelength

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dc.contributor.authorDe Barros M.H.P.
dc.contributor.authorKaufmann P.
dc.date.accessioned2024-03-13T01:48:15Z
dc.date.available2024-03-13T01:48:15Z
dc.date.issued1972
dc.description.abstractThe circular polarization from coronal condensations at λ = 4.3 cm correspond to the extraordinary mode of propagation, due to the contribution of preceding spots' polarities, being usually left-handed. The fewer cases of right-handed polarization are normally associated to an excess of sunspot plages in the southern hemisphere, thus making it difficult to give evidence for magnetoionic coupling phenomena as a general rule. © 1972 D. Reidel Publishing Company.
dc.description.firstpage203
dc.description.issuenumber1
dc.description.lastpage207
dc.description.volume27
dc.identifier.doi10.1007/BF00151784
dc.identifier.issn0038-0938
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/38107
dc.relation.ispartofSolar Physics
dc.rightsAcesso Restrito
dc.titleOn the long-term behaviour of the circular polarization from coronal condensation radio emission at 4.3 cm wavelength
dc.typeArtigo
local.scopus.citations2
local.scopus.eid2-s2.0-34250452420
local.scopus.updated2024-05-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=34250452420&origin=inward
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