Solar corona at centimetre wavelengths

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dc.contributor.authorKaufmann P.
dc.contributor.authorMatsuura O.T.
dc.date.accessioned2024-05-08T14:04:38Z
dc.date.available2024-05-08T14:04:38Z
dc.date.issued1968
dc.description.abstractDETAILED spectral information on the Sun in the range of wavelengths from near 3 cm to 21 cm was obtained on November 12, 1966, when total solar eclipse measurements were being made. Several observers, using accurate equipment, reported the residual solar emission during totality, and these data were used in a discussion of the cm-wavelength solar corona. In order to have some uniformity in the analysis, we first established a smoothed total solar flux spectrum for the period of November 11, 12 and 13 (as shown by Kaufmann1). The residuals, in percentages, uncorrected for the active regions present in the solar disk, were then transformed into flux units and are shown in Table 1. © 1968 Nature Publishing Group.
dc.description.firstpage921
dc.description.issuenumber5157
dc.description.lastpage922
dc.description.volume219
dc.identifier.doi10.1038/219921a0
dc.identifier.issn0028-0836
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/38698
dc.relation.ispartofNature
dc.rightsAcesso Restrito
dc.titleSolar corona at centimetre wavelengths
dc.typeCarta ao editor
local.scopus.citations2
local.scopus.eid2-s2.0-36949060857
local.scopus.updated2024-03-12
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=36949060857&origin=inward
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