Possible long-period oscillations in solar radio emission at microwaves

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dc.contributor.authorKaufmann P.
dc.date.accessioned2024-03-13T01:48:16Z
dc.date.available2024-03-13T01:48:16Z
dc.date.issued1972
dc.description.abstractLong-enduring bursts in the Sun at microwaves can occur in a succession, and rare examples of 41-min periodic structure are shown. The experimental difficulties for identifying such phenomena are discussed; their possible association with oscillations in quiescent prominences is suggested. © 1972 D. Reidel Publishing Company.
dc.description.firstpage178
dc.description.issuenumber1
dc.description.lastpage182
dc.description.volume23
dc.identifier.doi10.1007/BF00153901
dc.identifier.issn0038-0938
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/38108
dc.relation.ispartofSolar Physics
dc.rightsAcesso Restrito
dc.titlePossible long-period oscillations in solar radio emission at microwaves
dc.typeArtigo
local.scopus.citations9
local.scopus.eid2-s2.0-0040115836
local.scopus.updated2024-05-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=0040115836&origin=inward
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