Three years statistics of simple 3 solar bursts

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dc.contributor.authorMatsuura O.T.
dc.contributor.authorSantos P.M.D.
dc.date.accessioned2024-03-13T01:48:19Z
dc.date.available2024-03-13T01:48:19Z
dc.date.issued1971
dc.description.abstractA plasmoid may be ejected during a flare and condensed by a radiative instability. The spectral shape of the mean fluxes of Simple 3 (or long-enduring) solar events is interpreted in terms of a thermal emission from this transient condensation in the higher levels of the solar atmosphere. This condensation is thick enough to block the radiation from the underlying S-component. This explanation fits the observed polarization changes, as well as the thermal character of the bursts time profiles. A clue for solar activity forecasting as well as for detailed studies of active sources is indicated. © 1971 D. Reidel Publishing Company.
dc.description.firstpage402
dc.description.issuenumber2
dc.description.lastpage407
dc.description.volume17
dc.identifier.doi10.1007/BF00150043
dc.identifier.issn0038-0938
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/38111
dc.relation.ispartofSolar Physics
dc.rightsAcesso Restrito
dc.titleThree years statistics of simple 3 solar bursts
dc.typeArtigo
local.scopus.citations0
local.scopus.eid2-s2.0-34250450027
local.scopus.updated2024-05-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=34250450027&origin=inward
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