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dc.date.accessioned2022-06-21T15:04:39Z
dc.date.available2022-06-21T15:04:39Z
dc.date.created2022-06-09T17:24:39Z
dc.date.issued2022
dc.identifier.citationLabrosse, Nicolas Rodger, Andrew S. Radziszewski, Krzysztof Rudawy, Paweł Antolin, Patrick Fletcher, Lyndsay Levens, Peter J. Peat, Aaron W. Schmieder, Birgitte Simões, Paulo J.A. . First high resolution interferometric observation of a solar prominence with ALMA. Monthly Notices of the Royal Astronomical Society: Letters (MNRAS Letters). 2022, 513(1), L30-L34
dc.identifier.urihttp://hdl.handle.net/10852/94420
dc.description.abstractABSTRACT We present the first observation of a solar prominence at 84 − 116 GHz using the high resolution interferometric imaging of ALMA. Simultaneous observations in Hα from Białkaw Observatory and with SDO/AIA reveal similar prominence morphology to the ALMA observation. The contribution functions of 3 mm and Hα emission are shown to have significant overlap across a range of gas pressures. We estimate the maximum millimetre-continuum optical thickness to be τ3mm ≈ 2, and the brightness temperature from the observed Hα intensity. The brightness temperature measured by ALMA is ∼6000 – 7000 K in the prominence spine, which correlates well with the estimated brightness temperature for a kinetic temperature of 8000 K.
dc.languageEN
dc.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titleFirst high resolution interferometric observation of a solar prominence with ALMA
dc.title.alternativeENEngelskEnglishFirst high resolution interferometric observation of a solar prominence with ALMA
dc.typeJournal article
dc.creator.authorLabrosse, Nicolas
dc.creator.authorRodger, Andrew S.
dc.creator.authorRadziszewski, Krzysztof
dc.creator.authorRudawy, Paweł
dc.creator.authorAntolin, Patrick
dc.creator.authorFletcher, Lyndsay
dc.creator.authorLevens, Peter J.
dc.creator.authorPeat, Aaron W.
dc.creator.authorSchmieder, Birgitte
dc.creator.authorSimões, Paulo J.A.
cristin.unitcode185,15,3,40
cristin.unitnameRosseland senter for solfysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin2030594
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Monthly Notices of the Royal Astronomical Society: Letters (MNRAS Letters)&rft.volume=513&rft.spage=L30&rft.date=2022
dc.identifier.jtitleMonthly Notices of the Royal Astronomical Society: Letters (MNRAS Letters)
dc.identifier.volume513
dc.identifier.issue1
dc.identifier.startpageL30
dc.identifier.endpageL34
dc.identifier.doihttps://doi.org/10.1093/mnrasl/slac021
dc.identifier.urnURN:NBN:no-96962
dc.subject.nviVDP::Astrofysikk, astronomi: 438
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn1745-3925
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/94420/1/slac021.pdf
dc.type.versionPublishedVersion


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