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dc.date.accessioned2013-03-12T08:25:39Z
dc.date.available2013-03-12T08:25:39Z
dc.date.issued2010en_US
dc.date.submitted2010-06-01en_US
dc.identifier.citationGolding, Thomas Peter. Hydrogen ionization in 3d solar atmosphere models. Masteroppgave, University of Oslo, 2010en_US
dc.identifier.urihttp://hdl.handle.net/10852/10916
dc.description.abstractThe solar chromosphere is a region where the thermodynamics are out of equilibrium, and realistic values of temperature and electron densities here are difficult to obtain. Hydrogen, being the most abundant element in solar gas, dominates the equation of state. When doing time dependent multi-dimensional numeric modelling, the hydrogen state should therefore be treated with care - that means solving its rate equations. An algorithm that solves the rate equations with fixed radiative rates and couples hydrogen occupation numbers to the equation of state has been adjusted to fit the new stellar atmosphere code Bifrost. The method is described and results from a 3d test simulation are presented.eng
dc.language.isoengen_US
dc.subjectsolfysikk tilstandslikning magnetohydrodynamikk strålingstransporten_US
dc.titleHydrogen ionization in 3d solar atmosphere modelsen_US
dc.typeMaster thesisen_US
dc.date.updated2010-07-01en_US
dc.creator.authorGolding, Thomas Peteren_US
dc.subject.nsiVDP::438en_US
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:dissertation&rft.au=Golding, Thomas Peter&rft.title=Hydrogen ionization in 3d solar atmosphere models&rft.inst=University of Oslo&rft.date=2010&rft.degree=Masteroppgaveen_US
dc.identifier.urnURN:NBN:no-24881en_US
dc.type.documentMasteroppgaveen_US
dc.identifier.duo103225en_US
dc.contributor.supervisorMats Carlsson, Jorrit Leenaartsen_US
dc.identifier.bibsys101478534en_US
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/10916/1/golding_master2010.pdf


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