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A Statistical Inference Method for Interpreting the CLASP Observations

dc.date.accessioned2019-04-17T09:39:37Z
dc.date.available2019-04-17T09:39:37Z
dc.date.created2019-02-07T16:39:40Z
dc.date.issued2018
dc.identifier.citationStepan, Jiri Trujillo Bueno, J. Belluzzi, Luca Asensio Ramos, A. Manso Sainz, R. del Pino Aleman, T. Casini, Roberto Kano, Ryouhei Winebarger, Amy R. Auchère, Frédéric Ishikawa, Ryohko Narukage, Noriyuki Kobayashi, Ken Bando, Takamasa Katsukawa, Yukio Kubo, Masahito Ishikawa, Shin'nosuke Giono, Gabriel Hara, Hirohisa Suematsu, Yoshinori Shimizu, Toshifumi Sakao, Taro Tsuneta, Saku Ichimoto, Kiyoshi Cirtain, Jonathan W. Champey, Patrick R. De Pontieu, Bart Walter Carlsson, Mats . A Statistical Inference Method for Interpreting the CLASP Observations. Astrophysical Journal. 2018, 865:48
dc.identifier.urihttp://hdl.handle.net/10852/67708
dc.description.abstractOn 2015 September 3, the Chromospheric Lyman-Alpha SpectroPolarimeter (CLASP) successfully measured the linear polarization produced by scattering processes in the hydrogen Lyα line of the solar disk radiation, revealing conspicuous spatial variations in the Q/I and U/I signals. Via the Hanle effect, the line-center Q/I and U/I amplitudes encode information on the magnetic field of the chromosphere–corona transition region, but they are also sensitive to the three-dimensional structure of this corrugated interface region. With the help of a simple line-formation model, here we propose a statistical inference method for interpreting the Lyα line-center polarization observed by CLASP.en_US
dc.languageEN
dc.publisherUniversity of Chicago Press
dc.titleA Statistical Inference Method for Interpreting the CLASP Observationsen_US
dc.typeJournal articleen_US
dc.creator.authorStepan, Jiri
dc.creator.authorTrujillo Bueno, J.
dc.creator.authorBelluzzi, Luca
dc.creator.authorAsensio Ramos, A.
dc.creator.authorManso Sainz, R.
dc.creator.authordel Pino Aleman, T.
dc.creator.authorCasini, Roberto
dc.creator.authorKano, Ryouhei
dc.creator.authorWinebarger, Amy R.
dc.creator.authorAuchère, Frédéric
dc.creator.authorIshikawa, Ryohko
dc.creator.authorNarukage, Noriyuki
dc.creator.authorKobayashi, Ken
dc.creator.authorBando, Takamasa
dc.creator.authorKatsukawa, Yukio
dc.creator.authorKubo, Masahito
dc.creator.authorIshikawa, Shin'nosuke
dc.creator.authorGiono, Gabriel
dc.creator.authorHara, Hirohisa
dc.creator.authorSuematsu, Yoshinori
dc.creator.authorShimizu, Toshifumi
dc.creator.authorSakao, Taro
dc.creator.authorTsuneta, Saku
dc.creator.authorIchimoto, Kiyoshi
dc.creator.authorCirtain, Jonathan W.
dc.creator.authorChampey, Patrick R.
dc.creator.authorDe Pontieu, Bart Walter
dc.creator.authorCarlsson, Mats
cristin.unitcode185,15,3,40
cristin.unitnameRosseland senter for solfysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.cristin1674645
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Astrophysical Journal&rft.volume=865:48&rft.spage=&rft.date=2018
dc.identifier.jtitleAstrophysical Journal
dc.identifier.volume865:48
dc.identifier.pagecount11
dc.identifier.doihttp://dx.doi.org/10.3847/1538-4357/aad910
dc.identifier.urnURN:NBN:no-70894
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn0004-637X
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/67708/1/%25C5%25A0t%25C4%259Bp%25C3%25A1n_2018_ApJ_865_48.pdf
dc.type.versionPublishedVersion
cristin.articleid48
dc.relation.projectNFR/262622


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