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dc.contributorInstitute for Astronomy, Astrophysics, Space Applications and Remote Sensing (IAASARS), National Observatory of Athens, 15236, Penteli, Greece
dc.contributorTrinity College Dublin, College Green, Dublin 2, Ireland
dc.contributorArmagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland
dc.contributor.authorPark, S. -H.
dc.contributor.authorTsiropoula, G.
dc.contributor.authorKontogiannis, I.
dc.contributor.authorTziotziou, K.
dc.contributor.authorScullion, E.
dc.contributor.authorDoyle, J. G.
dc.date.accessioned2024-02-21T11:03:08Z
dc.date.available2024-02-21T11:03:08Z
dc.date.issued2016-02-01T00:00:00Z
dc.identifier.doi10.1051/0004-6361/201527440
dc.identifier.doi10.48550/arXiv.1512.06032
dc.identifier.other2015arXiv151206032P
dc.identifier.otherastro-ph.SR
dc.identifier.other10.1051/0004-6361/201527440
dc.identifier.other2015arXiv151206032P
dc.identifier.other2016A&A...586A..25P
dc.identifier.otherarXiv:1512.06032
dc.identifier.other10.48550/arXiv.1512.06032
dc.identifier.other-
dc.identifier.urihttp://hdl.handle.net/20.500.14302/1761
dc.description.abstractContext. Ubiquitous small-scale vortices have recently been found in the lower atmosphere of the quiet Sun in state-of-the-art solar observations and in numerical simulations. <BR /> Aims: We investigate the characteristics and temporal evolution of a granular-scale vortex and its associated upflows through the photosphere and chromosphere of a quiet Sun internetwork region. <BR /> Methods: We analyzed high spatial and temporal resolution ground- and spaced-based observations of a quiet Sun region. The observations consist of high-cadence time series of wideband and narrowband images of both Hα 6563 Å and Ca II 8542 Å lines obtained with the CRisp Imaging SpectroPolarimeter (CRISP) instrument at the Swedish 1-m Solar Telescope (SST), as well as ultraviolet imaging and spectral data simultaneously obtained by the Interface Region Imaging Spectrograph (IRIS). <BR /> Results: A small-scale vortex is observed for the first time simultaneously in Hα, Ca II 8542 Å, and Mg II k lines. During the evolution of the vortex, Hα narrowband images at -0.77 Å and Ca II 8542 Å narrowband images at -0.5 Å, and their corresponding Doppler signal maps, clearly show consecutive high-speed upflow events in the vortex region. These high-speed upflows with a size of 0.5-1 Mm appear in the shape of spiral arms and exhibit two distinctive apparent motions in the plane of sky for a few minutes: (1) a swirling motion with an average speed of 13 km s<SUP>-1</SUP> and (2) an expanding motion at a rate of 4-6 km s<SUP>-1</SUP>. Furthermore, the spectral analysis of Mg II k and Mg II subordinate lines in the vortex region indicates an upward velocity of up to ~8 km s<SUP>-1</SUP> along with a higher temperature compared to the nearby quiet Sun chromosphere. <BR /> Conclusions: The consecutive small-scale vortex events can heat the upper chromosphere by driving continuous high-speed upflows through the lower atmosphere. <P />Movies associated to Figs. 2 and 3 are available at <A href=http://www.aanda.org/10.1051/0004-6361/201527440/olm>http://www.aanda.org</A>
dc.publisherAstronomy and Astrophysics
dc.titleFirst simultaneous SST/CRISP and IRIS observations of a small-scale quiet Sun vortex
dc.typearticle
dc.source.journalA&A
dc.source.journalA&A...586
dc.source.volume586
refterms.dateFOA2024-02-21T11:03:08Z
dc.identifier.bibcode2016A&A...586A..25P


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