Modeling the Solar Chromosphere

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dc.creatorCarlsson, M.
dc.date2007-04-11
dc.date.accessioned2026-07-07T07:56:18Z
dc.date.available2026-07-07T07:56:18Z
dc.descriptionSpectral diagnostic features formed in the solar chromosphere are few and difficult to interpret -- they are neither formed in the optically thin regime nor in local thermodynamic equilibrium (LTE). To probe the state of the chromosphere, both from observations and theory, it is therefore necessary with modeling. I discuss both traditional semi-empirical modeling, numerical experiments illustrating important ingredients necessary for a self-consistent theoretical modeling of the solar chromosphere and the first results of such models.
dc.description15 pages, In press,"Physics of Chromospheric Plasmas" (Coimbra), ASP 368, 49 (2007)
dc.identifierhttps://arxiv.org/abs/0704.1509
dc.identifierhttp://arxiv.org/abs/0704.1509
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/127261
dc.subjectAstrophysics
dc.titleModeling the Solar Chromosphere
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