Some characteristics of an S-component of solar radiation identified on November 1966 eclipse at 4.28-cm wavelength

Página do item simplificado
dc.contributor.authorKaufmann P.
dc.date.accessioned2024-05-08T14:04:40Z
dc.date.available2024-05-08T14:04:40Z
dc.date.issued1968
dc.description.abstractA strong S-component of solar radiation was identified during the total solar eclipse of November 12, 1966. Its characteristics, as measured at 4.28 cm, were studied in terms of flux and polarization, and its spectral features were derived by the use of data from other observatories. The whole source presented approximately the typical characteristics suggested by some authors in the last few years, and further it has been shown that it could be resolved into at least two enhanced regions, one showing unpolarized radiation with a brightness temperature Tb≈ 1.2 × 106 °K, and the other showing 50% of left-handed circularly polarized radiation, with Tb≈ 0.7 × 106 °K. The source's overall characteristics favour the presence of non-thermal absorption at the emitting regions. © 1968 D. Reidel Publishing Company.
dc.description.firstpage58
dc.description.issuenumber1
dc.description.lastpage66
dc.description.volume4
dc.identifier.doi10.1007/BF00146998
dc.identifier.issn0038-0938
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/38700
dc.relation.ispartofSolar Physics
dc.rightsAcesso Restrito
dc.titleSome characteristics of an S-component of solar radiation identified on November 1966 eclipse at 4.28-cm wavelength
dc.typeArtigo
local.scopus.citations6
local.scopus.eid2-s2.0-22344440244
local.scopus.updated2024-03-12
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=22344440244&origin=inward
Arquivos
Coleções
Artigos de periódico