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dc.contributor.authorTesta, Paola
dc.contributor.authorDe Pontieu, Bart
dc.contributor.authorAllred, J.
dc.contributor.authorCarlsson, Mats
dc.contributor.authorReale, F.
dc.contributor.authorDaw, A.
dc.contributor.authorHansteen, Viggo H.
dc.contributor.authorMartinez-Sykora, J.
dc.contributor.authorLiu, W.
dc.contributor.authorDeLuca, E.E.
dc.contributor.authorGolub, Leon
dc.contributor.authorMcKillop, Sean
dc.contributor.authorReeves, Kathy K.
dc.contributor.authorSaar, Steven
dc.contributor.authorTian, Hui
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.authorKleint, Lucia
dc.contributor.authorKankelborg, Charles
dc.contributor.authorJaeggli, Sarah
dc.date.accessioned2015-03-23T20:46:58Z
dc.date.available2015-03-23T20:46:58Z
dc.date.issued2014-10
dc.identifier.citationTesta, P., B. De Pontieu, J. Allred, M. Carlsson, F. Reale, A. Daw, V. Hansteen, J. Martinez-Sykora, W. Liu, E.E. DeLuca, L. Golub, S. McKillop, K. Reeves, S. Saar, H. Tian, J. Lemen, A. Title, P. Boerner, N. Hurlburt, T.D. Tarbell, J.P. Wuelser, L. Kleint, C. Kankelborg, S. Jaeggli. "Evidence of nonthermal particles in coronal loops heated impulsively by nanoflares." Science 346, no. 6207 (2014): 1255724. http://dx.doi.org/10.1126/science.1255724en_US
dc.identifier.issn0036-8075
dc.identifier.urihttps://scholarworks.montana.edu/xmlui/handle/1/8939
dc.description.abstractThe physical processes causing energy exchange between the Sun’s hot corona and its cool lower atmosphere remain poorly understood. The chromosphere and transition region (TR) form an interface region between the surface and the corona that is highly sensitive to the coronal heating mechanism. High-resolution observations with the Interface Region Imaging Spectrograph (IRIS) reveal rapid variability (~20 to 60 seconds) of intensity and velocity on small spatial scales (≲500 kilometers) at the footpoints of hot and dynamic coronal loops. The observations are consistent with numerical simulations of heating by beams of nonthermal electrons, which are generated in small impulsive (≲30 seconds) heating events called “coronal nanoflares.” The accelerated electrons deposit a sizable fraction of their energy (≲1025 erg) in the chromosphere and TR. Our analysis provides tight constraints on the properties of such electron beams and new diagnostics for their presence in the nonflaring corona.en_US
dc.subjectAstrophysicsen_US
dc.titleEvidence of nonthermal particles in coronal loops heated impulsively by nanoflaresen_US
dc.typeArticleen_US
mus.citation.extentfirstpage1255724en_US
mus.citation.issue6207en_US
mus.citation.journaltitleScienceen_US
mus.citation.volume346en_US
mus.identifier.categoryPhysics & Mathematicsen_US
mus.identifier.doi10.1126/science.1255724en_US
mus.relation.collegeCollege of Letters & Scienceen_US
mus.relation.collegeCollege of Letters & Science
mus.relation.departmentPhysics.en_US
mus.relation.universityMontana State University - Bozemanen_US


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