Coherent Synchrotron Radiation in Laboratory Accelerators and the Double-Spectral Feature in Solar Flares

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dc.contributor.authorCruz W.
dc.contributor.authorSzpigel S.
dc.contributor.authorKaufmann P.
dc.contributor.authorRaulin J.-P.
dc.contributor.authorKlopf M.
dc.date.accessioned2024-03-13T00:54:36Z
dc.date.available2024-03-13T00:54:36Z
dc.date.issued2016
dc.description.abstractCopyright © 2017 International Astronomical Union.Recent observations of solar flares at high-frequencies have provided evidence of a new spectral component with fluxes increasing with frequency in the sub-THz to THz range. This new component occurs simultaneously but is separated from the well-known microwave spectral component that maximizes at frequencies of a few to tens of GHz. The aim of this work is to study in detail a mechanism recently suggested to describe the double-spectrum feature observed in solar flares based on the physical process known as microbunching instability, which occurs with high-energy electron beams in laboratory accelerators.
dc.description.firstpage134
dc.description.lastpage136
dc.description.volume12
dc.identifier.doi10.1017/S1743921317003787
dc.identifier.issn1743-9221
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/36051
dc.relation.ispartofProceedings of the International Astronomical Union
dc.rightsAcesso Aberto
dc.subject.otherlanguageCoherent synchrotron radiation
dc.subject.otherlanguageMicrobunching instability
dc.subject.otherlanguageSolar flares
dc.titleCoherent Synchrotron Radiation in Laboratory Accelerators and the Double-Spectral Feature in Solar Flares
dc.typeArtigo de evento
local.scopus.citations0
local.scopus.eid2-s2.0-85030097630
local.scopus.updated2024-05-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85030097630&origin=inward
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