The impulsiveness of microwave bursts and its association with sunspot types

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dc.contributor.authorMatsuura O.T.
dc.contributor.authorNave M.F.F.
dc.date.accessioned2024-03-13T01:48:20Z
dc.date.available2024-03-13T01:48:20Z
dc.date.issued1971
dc.description.abstractA statistical analysis on 220 impulsive microwave bursts showed a marked preference to occur in sunspots of type D, E and F (after Zürich classification). Assuming a shock mechanism for accelerating electrons, this tendency seems to be related to the size of the magnetic loops. © 1971 D. Reidel Publishing Company.
dc.description.firstpage417
dc.description.issuenumber2
dc.description.lastpage422
dc.description.volume16
dc.identifier.doi10.1007/BF00162484
dc.identifier.issn0038-0938
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/38112
dc.relation.ispartofSolar Physics
dc.rightsAcesso Restrito
dc.titleThe impulsiveness of microwave bursts and its association with sunspot types
dc.typeArtigo
local.scopus.citations0
local.scopus.eid2-s2.0-34250450699
local.scopus.updated2024-05-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=34250450699&origin=inward
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