dc.date.accessioned | 2020-05-22T18:17:20Z | |
dc.date.available | 2020-11-27T23:46:04Z | |
dc.date.created | 2020-01-27T15:15:33Z | |
dc.date.issued | 2019 | |
dc.identifier.citation | Rutten, Robert . Non-Equilibrium Spectrum Formation Affecting Solar Irradiance. Solar Physics. 2019, 294 | |
dc.identifier.uri | http://hdl.handle.net/10852/76092 | |
dc.description.abstract | This is an overview of non-equilibrium aspects of the formation of solar continua and lines affecting the contributions by magnetic network and plage to spectrally resolved solar irradiance. After a brief summary of these contributions and a compact refresher of solar spectrum formation, the emphasis is on graphical exposition. Major obstacles for simulation-based irradiance studies are how to cope with NLTE scattering in the violet and ultraviolet line haze and how to cope with retarded hydrogen opacities in infrared and mm radiation. | |
dc.language | EN | |
dc.title | Non-Equilibrium Spectrum Formation Affecting Solar Irradiance | |
dc.type | Journal article | |
dc.creator.author | Rutten, Robert | |
cristin.unitcode | 185,15,3,40 | |
cristin.unitname | Rosseland senter for solfysikk | |
cristin.ispublished | true | |
cristin.fulltext | postprint | |
cristin.qualitycode | 1 | |
dc.identifier.cristin | 1783304 | |
dc.identifier.bibliographiccitation | info:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Solar Physics&rft.volume=294&rft.spage=&rft.date=2019 | |
dc.identifier.jtitle | Solar Physics | |
dc.identifier.volume | 294 | |
dc.identifier.issue | 11 | |
dc.identifier.pagecount | 23 | |
dc.identifier.doi | https://doi.org/10.1007/s11207-019-1535-2 | |
dc.identifier.urn | URN:NBN:no-79200 | |
dc.type.document | Tidsskriftartikkel | |
dc.type.peerreviewed | Peer reviewed | |
dc.source.issn | 0038-0938 | |
dc.identifier.fulltext | Fulltext https://www.duo.uio.no/bitstream/handle/10852/76092/1/1908.04624.pdf | |
dc.type.version | AcceptedVersion | |
cristin.articleid | 165 | |
dc.relation.project | NFR/262622 | |