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Statements

Subject Item
n2:RIV%2F67985815%3A_____%2F12%3A00386505%21RIV13-GA0-67985815
rdf:type
skos:Concept n13:Vysledek
dcterms:description
In the context of interpreting non-thermal hard X-ray emission and γ lines emanating from the footpoints of flare loops, most contemporary flare models assign a fundamental role during the flare energy release, transport and deposition to the high energy non-thermal particle beams. In this contribution we concentrate on modelling of the spectroscopic properties of chromospheric flare emission in optical hydrogen lines generated due to the bombardment of the chromosphere and photosphere by neutral beams with power-law spectra. In order to obtain an estimate of the neutral beam flare heating in the solar atmosphere we produced a simple model describing the propagation and thermalisation of neutral beams. We compare the neutral beam flare heating with the flare heating produced by corresponding pure electron and proton beams. Further we compare the contribution functions for Hα line obtained for neutral and electron beam heating. In the context of interpreting non-thermal hard X-ray emission and γ lines emanating from the footpoints of flare loops, most contemporary flare models assign a fundamental role during the flare energy release, transport and deposition to the high energy non-thermal particle beams. In this contribution we concentrate on modelling of the spectroscopic properties of chromospheric flare emission in optical hydrogen lines generated due to the bombardment of the chromosphere and photosphere by neutral beams with power-law spectra. In order to obtain an estimate of the neutral beam flare heating in the solar atmosphere we produced a simple model describing the propagation and thermalisation of neutral beams. We compare the neutral beam flare heating with the flare heating produced by corresponding pure electron and proton beams. Further we compare the contribution functions for Hα line obtained for neutral and electron beam heating.
dcterms:title
Formation of Balmer Lines in Impulsively Heated Flare Atmosphere by Neutral Beams Formation of Balmer Lines in Impulsively Heated Flare Atmosphere by Neutral Beams
skos:prefLabel
Formation of Balmer Lines in Impulsively Heated Flare Atmosphere by Neutral Beams Formation of Balmer Lines in Impulsively Heated Flare Atmosphere by Neutral Beams
skos:notation
RIV/67985815:_____/12:00386505!RIV13-GA0-67985815
n13:predkladatel
n14:ico%3A67985815
n3:aktivita
n12:Z n12:P
n3:aktivity
P(GA205/07/1100), P(GAP209/10/1680), P(GP205/06/P135), Z(AV0Z10030501)
n3:dodaniDat
n11:2013
n3:domaciTvurceVysledku
n8:9659455 n8:9031006 n8:3741451
n3:druhVysledku
n18:D
n3:duvernostUdaju
n5:S
n3:entitaPredkladatele
n17:predkladatel
n3:idSjednocenehoVysledku
136995
n3:idVysledku
RIV/67985815:_____/12:00386505
n3:jazykVysledku
n19:eng
n3:klicovaSlova
solar atmoshpere; neutral beams
n3:klicoveSlovo
n7:neutral%20beams n7:solar%20atmoshpere
n3:kontrolniKodProRIV
[E769DB6E914E]
n3:mistoKonaniAkce
Tokyo
n3:mistoVydani
San Francisco
n3:nazevZdroje
Hinode-3: The 3rd Hinode Science Meeting
n3:obor
n16:BN
n3:pocetDomacichTvurcuVysledku
3
n3:pocetTvurcuVysledku
5
n3:projekt
n15:GP205%2F06%2FP135 n15:GAP209%2F10%2F1680 n15:GA205%2F07%2F1100
n3:rokUplatneniVysledku
n11:2012
n3:tvurceVysledku
Karlický, Marian Heinzel, Petr Kašparová, Jana Moravec, Z. Varady, M.
n3:typAkce
n22:WRD
n3:zahajeniAkce
2009-12-01+01:00
n3:zamer
n10:AV0Z10030501
s:numberOfPages
4
n20:hasPublisher
Astronomical Society otf the Pacific
n4:isbn
9781583817902