Halpha with Heating by Particle Beams

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dc.creatorKasparova, J.
dc.creatorVarady, M.
dc.creatorKarlicky, M.
dc.creatorHeinzel, P.
dc.creatorMoravec, Z.
dc.date2007-03-30
dc.date.accessioned2026-07-07T11:01:19Z
dc.date.available2026-07-07T11:01:19Z
dc.descriptionUsing 1D NLTE radiative hydrodynamics we model the influence of the particle beams on the Halpha line profile treating the beam propagation and the atmosphere evolution self-consistently. We focus on the influence of the non-thermal collisional rates and the return current. Based on our results, we propose a diagnostic method for determination of the particle beam presence in the formation regions of the Halpha line.
dc.descriptionIn press, "Physics of Chromospheric Plasmas" (Coimbra), ASP 368, 441 (2007)
dc.identifierhttps://arxiv.org/abs/astro-ph/0703800
dc.identifierhttp://arxiv.org/abs/astro-ph/0703800
dc.identifierASPConf.Ser.368:27,2007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/187919
dc.subjectAstrophysics
dc.titleHalpha with Heating by Particle Beams
dc.typetext

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