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Can the Superposition of Evaporative Flows Explain Broad Fe XXI Profiles during Solar Flares?

dc.date.accessioned2020-04-11T19:25:27Z
dc.date.available2020-04-11T19:25:27Z
dc.date.created2019-10-10T17:48:14Z
dc.date.issued2019
dc.identifier.citationPolito, Vanessa Testa, Paola De Pontieu, Bart Walter . Can the Superposition of Evaporative Flows Explain Broad Fe XXI Profiles during Solar Flares?. Astrophysical Journal Letters. 2019, 879(2)
dc.identifier.urihttp://hdl.handle.net/10852/74494
dc.languageEN
dc.publisherInstitute of Physics Publishing Ltd.
dc.titleCan the Superposition of Evaporative Flows Explain Broad Fe XXI Profiles during Solar Flares?
dc.typeJournal article
dc.creator.authorPolito, Vanessa
dc.creator.authorTesta, Paola
dc.creator.authorDe Pontieu, Bart Walter
cristin.unitcode185,15,3,40
cristin.unitnameRosseland senter for solfysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.cristin1736218
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 Letters&rft.volume=879&rft.spage=&rft.date=2019
dc.identifier.jtitleAstrophysical Journal Letters
dc.identifier.volume879
dc.identifier.issue2
dc.identifier.pagecount8
dc.identifier.doihttps://doi.org/10.3847/2041-8213/ab290b
dc.identifier.urnURN:NBN:no-77605
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn2041-8205
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/74494/1/Polito_2019_ApJL_879_L17.pdf
dc.type.versionPublishedVersion
cristin.articleidL17
dc.relation.projectNFR/251369
dc.relation.projectNFR/262622


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