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dc.date.accessioned2017-08-14T12:50:36Z
dc.date.available2017-08-14T12:50:36Z
dc.date.created2015-08-17T11:25:04Z
dc.date.issued2015
dc.identifier.citationMendes Domingos Pereira, Tiago Carlsson, Mats De Pontieu, Bart Walter Hansteen, Viggo . THE FORMATION of IRIS DIAGNOSTICS. IV. the Mg ii TRIPLET LINES AS A NEW DIAGNOSTIC FOR LOWER CHROMOSPHERIC HEATING. The Astrophysical Journal. 2015, 806(1)
dc.identifier.urihttp://hdl.handle.net/10852/56978
dc.description.abstractA triplet of subordinate lines of Mg ii exists in the region around the h&k lines. In solar spectra these lines are seen mostly in absorption, but in some cases can become emission lines. The aim of this work is to study the formation of this triplet, and investigate any diagnostic value they can bring. Using 3D radiative magnetohydrodynamic simulations of quiet Sun and flaring flux emergence, we synthesize spectra and investigate how spectral features respond to the underlying atmosphere. Reproduced with permission from the Astrophysical Journal. © IOP Publishingen_US
dc.languageEN
dc.publisherUniversity of Chicago Press
dc.titleTHE FORMATION of IRIS DIAGNOSTICS. IV. the Mg ii TRIPLET LINES AS A NEW DIAGNOSTIC FOR LOWER CHROMOSPHERIC HEATINGen_US
dc.typeJournal articleen_US
dc.creator.authorMendes Domingos Pereira, Tiago
dc.creator.authorCarlsson, Mats
dc.creator.authorDe Pontieu, Bart Walter
dc.creator.authorHansteen, Viggo
cristin.unitcode185,15,3,0
cristin.unitnameInstitutt for teoretisk astrofysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.cristin1258324
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=The Astrophysical Journal&rft.volume=806&rft.spage=&rft.date=2015
dc.identifier.jtitleThe Astrophysical Journal
dc.identifier.volume806
dc.identifier.issue1
dc.identifier.pagecount8
dc.identifier.doihttp://dx.doi.org/10.1088/0004-637X/806/1/14
dc.identifier.urnURN:NBN:no-59726
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn0004-637X
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/56978/1/Pereira_2015_ApJ_806_14.pdf
dc.type.versionPublishedVersion
cristin.articleid14


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