Solar radio emissions

dc.contributor.authorRaulin J.-P.
dc.contributor.authorPacini A.A.
dc.date.accessioned2024-03-13T01:44:30Z
dc.date.available2024-03-13T01:44:30Z
dc.date.issued2005
dc.description.abstractIn this paper, we present a tutorial review which was presented at the first Advanced School on Space Environment (ASSE 2004). We first describe the basics of radioastronomy definitions, and discuss radiation processes relevant to solar radio emissions like plasma emission, free-free bremsstrählung and gyromagnetic emissions. We illustrate these fundamentals by describing recent solar radio observations and the constraints they bring on different solar physical parameters. We focus on solar radio emissions from the quiet sun, active regions and during explosive events known as solar flares, and how the latter can bring quantitative informations on the particles responsible for the emission. Finally, particular attention is paid to new radio diagnostics obtained at very high frequencies in the millimeter/submillimeter range, as well as to radio emissions relevant to Space Weather studies. © 2005 COSPAR. Published by Elsevier Ltd. All rights reserved.
dc.description.firstpage739
dc.description.issuenumber5
dc.description.lastpage754
dc.description.volume35
dc.identifier.doi10.1016/j.asr.2005.03.138
dc.identifier.issn0273-1177
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/37901
dc.relation.ispartofAdvances in Space Research
dc.rightsAcesso Restrito
dc.subject.otherlanguageRadiation mechanisms
dc.subject.otherlanguageSolar flares
dc.subject.otherlanguageSolar radio astronomy
dc.subject.otherlanguageSubmillimeter waves
dc.titleSolar radio emissions
dc.typeArtigo de evento
local.scopus.citations27
local.scopus.eid2-s2.0-20744439133
local.scopus.subjectRadiation mechanisms
local.scopus.subjectSolar flares
local.scopus.subjectSolar radio astronomy
local.scopus.subjectSolar surfaces
local.scopus.updated2024-05-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=20744439133&origin=inward
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