Changes in coronal condensations emission after solar bursts at microwaves

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dc.contributor.authorKaufmann P.
dc.contributor.authorScalise Jr. E.
dc.contributor.authorSantos P.M.D.
dc.date.accessioned2024-03-13T01:48:24Z
dc.date.available2024-03-13T01:48:24Z
dc.date.issued1970
dc.description.abstractThe amount of circular polarization of the total solar radio emission at 7 GHz present permanent changes after the occurrence of certain radio bursts associated with larger flares. For isolated S-components, associated with such flares the changes of the polarization degree ΔΠsranges between 0.004 to 0.1, and appears to be a function of the flare importance. A semi-qualitative interpretation associates ΔΠswith magnetic field reductions at the S-component, agreeing fairly well with a flare mechanism based on collisionless dissipation of magnetic energy, corresponding to energies in the range of 1030 to 1032 ergs, assuming an average model for the coronal condensations. © 1970 D. Reidel Publishing Company.
dc.description.firstpage195
dc.description.issuenumber1
dc.description.lastpage201
dc.description.volume15
dc.identifier.doi10.1007/BF00149485
dc.identifier.issn0038-0938
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/38116
dc.relation.ispartofSolar Physics
dc.rightsAcesso Restrito
dc.titleChanges in coronal condensations emission after solar bursts at microwaves
dc.typeArtigo
local.scopus.citations1
local.scopus.eid2-s2.0-34250482709
local.scopus.updated2024-05-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=34250482709&origin=inward
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