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dc.contributor.authorDe Pontieu, Bart
dc.contributor.authorRouppe van der Voort, L.
dc.contributor.authorMcIntosh, Scott W.
dc.contributor.authorPereira, Tiago M. D.
dc.contributor.authorCarlsson, Mats
dc.contributor.authorHansteen, Viggo H.
dc.contributor.authorSkogsrud, H.
dc.contributor.authorLemen, James
dc.contributor.authorTitle, Alan M.
dc.contributor.authorBoerner, P.
dc.contributor.authorHurlburt, Neal E.
dc.contributor.authorTarbell, Ted D.
dc.contributor.authorWuelser, Jean-Pierre
dc.contributor.authorDeLuca, E.E.
dc.contributor.authorGolub, Leon
dc.contributor.authorMcKillop, Sean
dc.contributor.authorReeves, Kathy K.
dc.contributor.authorSaar, Steven
dc.contributor.authorTesta, Paola
dc.contributor.authorTian, Hui
dc.contributor.authorKankelborg, Charles
dc.contributor.authorJaeggli, Sarah
dc.contributor.authorKleint, Lucia
dc.contributor.authorMartinez-Sykora, J.
dc.date.accessioned2015-03-23T21:09:01Z
dc.date.available2015-03-23T21:09:01Z
dc.date.issued2014-10
dc.identifier.citationDe Pontieu, B., L. Rouppe van der Voort, S. W. McIntosh, T. M. D. Pereira, M. Carlsson, V. Hansteen, H. Skogsrud, et al. "On the Prevalence of Small-Scale Twist in the Solar Chromosphere and Transition Region." Science 346, no. 6207 (October 16, 2014): 1255732–1255732. doi:10.1126/science.1255732.en_US
dc.identifier.issn0036-8075
dc.identifier.urihttps://scholarworks.montana.edu/xmlui/handle/1/8942
dc.description.abstractThe solar chromosphere and transition region (TR) form an interface between the Sun’s surface and its hot outer atmosphere. There, most of the nonthermal energy that powers the solar atmosphere is transformed into heat, although the detailed mechanism remains elusive. High-resolution (0.33–arc second) observations with NASA’s Interface Region Imaging Spectrograph (IRIS) reveal a chromosphere and TR that are replete with twist or torsional motions on sub–arc second scales, occurring in active regions, quiet Sun regions, and coronal holes alike. We coordinated observations with the Swedish 1-meter Solar Telescope (SST) to quantify these twisting motions and their association with rapid heating to at least TR temperatures. This view of the interface region provides insight into what heats the low solar atmosphere.en_US
dc.publisherDe Pontieu, B., L. Rouppe van der Voort, S. W. McIntosh, T. M. D. Pereira, M. Carlsson, V. Hansteen, H. Skogsrud, et al. “On the Prevalence of Small-Scale Twist in the Solar Chromosphere and Transition Region.” Science 346, no. 6207 (October 16, 2014): 1255732–1255732. doi:10.1126/science.1255732.en_US
dc.subjectAstrophysicsen_US
dc.titleOn the prevalence of small-scale twist in the solar chromosphere and transition regionen_US
dc.typeArticleen_US
mus.citation.extentfirstpage1255732en_US
mus.citation.issue6207en_US
mus.citation.journaltitleScienceen_US
mus.citation.volume346en_US
mus.identifier.categoryPhysics & Mathematicsen_US
mus.identifier.doi10.1126/science.1255732en_US
mus.relation.collegeCollege of Letters & Science
mus.relation.collegeCollege of Letters & Scienceen_US
mus.relation.departmentPhysics.en_US
mus.relation.universityMontana State University - Bozemanen_US


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