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Statements

Subject Item
n2:RIV%2F67985815%3A_____%2F12%3A00386857%21RIV13-GA0-67985815
rdf:type
skos:Concept n12:Vysledek
dcterms:description
Spectral continua observed during solar flares may contain information about both thermal and non-thermal heating mechanisms. Using two semi-empirical flare models F2 and FLA, we synthesize the thermal continua from optical to mm–radio domains and compare their intensities with quiet-Sun values computed from a recent model C7. In this way, the far-infrared and sub-mm/mm continua are studied for the first time, and we present our results as a benchmark for further modeling and for planning new observations, especially with the ALMA instrument. Finally, we demonstrate how these continua are formed and show a close correspondence between their brightness temperature and the kinetic-temperature structure of the flaring atmosphere. Spectral continua observed during solar flares may contain information about both thermal and non-thermal heating mechanisms. Using two semi-empirical flare models F2 and FLA, we synthesize the thermal continua from optical to mm–radio domains and compare their intensities with quiet-Sun values computed from a recent model C7. In this way, the far-infrared and sub-mm/mm continua are studied for the first time, and we present our results as a benchmark for further modeling and for planning new observations, especially with the ALMA instrument. Finally, we demonstrate how these continua are formed and show a close correspondence between their brightness temperature and the kinetic-temperature structure of the flaring atmosphere.
dcterms:title
Optical-to-Radio Continua in Solar Flares Optical-to-Radio Continua in Solar Flares
skos:prefLabel
Optical-to-Radio Continua in Solar Flares Optical-to-Radio Continua in Solar Flares
skos:notation
RIV/67985815:_____/12:00386857!RIV13-GA0-67985815
n12:predkladatel
n13:ico%3A67985815
n3:aktivita
n7:P n7:Z
n3:aktivity
P(GAP209/10/1680), Z(AV0Z10030501)
n3:cisloPeriodika
1
n3:dodaniDat
n19:2013
n3:domaciTvurceVysledku
n20:3741451
n3:druhVysledku
n8:J
n3:duvernostUdaju
n17:S
n3:entitaPredkladatele
n18:predkladatel
n3:idSjednocenehoVysledku
156767
n3:idVysledku
RIV/67985815:_____/12:00386857
n3:jazykVysledku
n11:eng
n3:klicovaSlova
solar flares; spectral continua; diagnostics
n3:klicoveSlovo
n5:spectral%20continua n5:solar%20flares n5:diagnostics
n3:kodStatuVydavatele
NL - Nizozemsko
n3:kontrolniKodProRIV
[7A470FB4884C]
n3:nazevZdroje
Solar Physics
n3:obor
n15:BN
n3:pocetDomacichTvurcuVysledku
1
n3:pocetTvurcuVysledku
2
n3:projekt
n16:GAP209%2F10%2F1680
n3:rokUplatneniVysledku
n19:2012
n3:svazekPeriodika
227
n3:tvurceVysledku
Heinzel, Petr Avrett, E. H.
n3:wos
000299770300004
n3:zamer
n9:AV0Z10030501
s:issn
0038-0938
s:numberOfPages
14
n14:doi
10.1007/s11207-011-9823-5