Wavelet decomposition of submillimeter solar radio bursts

Página do item simplificado
dc.contributor.authorMakhmutov V.S.
dc.contributor.authorRaulin J.-P.
dc.contributor.authorGimenez De Castro C.G.
dc.contributor.authorKaufmann P.
dc.contributor.authorCorreia E.
dc.date.accessioned2024-03-13T01:45:58Z
dc.date.available2024-03-13T01:45:58Z
dc.date.issued2003
dc.description.abstractWe present the results of wavelet decomposition of fast-time structures during four solar flares observed by the Solar Submillimeter-wave Telescope at 212 GHz. The result of the analysis shows (1) observational evidence on the existence of submm-emission time variations in the range from a few tens of millisecond up to few seconds during solar flares, and (2) that when a solar flare is in progress the time scales reduce as the bulk of the emission flux time variations is increasing.
dc.description.firstpage211
dc.description.issuenumber1-2
dc.description.lastpage220
dc.description.volume218
dc.identifier.doi10.1023/b:sola.0000013047.26419.33
dc.identifier.issn0038-0938
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/37983
dc.relation.ispartofSolar Physics
dc.rightsAcesso Restrito
dc.titleWavelet decomposition of submillimeter solar radio bursts
dc.typeArtigo
local.scopus.citations12
local.scopus.eid2-s2.0-3543089143
local.scopus.updated2024-05-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=3543089143&origin=inward
Arquivos
Coleções
Artigos de periódico