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dc.contributor.authorLi, Ying
dc.contributor.authorKelly, Madie
dc.contributor.authorDing, M. D.
dc.contributor.authorQiu, Jiong
dc.contributor.authorZhu, X. S.
dc.contributor.authorGan, W. Q.
dc.date.accessioned2018-04-26T16:26:16Z
dc.date.available2018-04-26T16:26:16Z
dc.date.issued2017-10
dc.identifier.citationLi, Y., M. Kelly, M. D. Ding, J. Qiu, X. S. Zhu, and W. Q. Gan. "Spectroscopic Observations of Magnetic Reconnection and Chromospheric Evaporation in an X-shaped Solar Flare." ASTROPHYSICAL JOURNAL 848, no. 2 (October 2017). DOI: 10.3847/1538-4357/aa89e4.en_US
dc.identifier.issn0004-637X
dc.identifier.urihttps://scholarworks.montana.edu/xmlui/handle/1/14519
dc.description.abstractWe present observations of distinct UV spectral properties at different locations during an atypical X-shaped flare (SOL2014-11-09T15:32) observed by the Interface Region Imaging Spectrograph (IRIS). In this flare, four chromospheric ribbons appear and converge at an X-point where a separator is anchored. Above the X-point, two sets of non-coplanar coronal loops approach laterally and reconnect at the separator. The IRIS. slit was located close to the X-point, cutting across some of the flare ribbons and loops. Near the location of the separator, the Si IV 1402.77 angstrom line exhibits significantly broadened line wings extending to 200 km s(-1) with an unshifted line core. These spectral features suggest the presence of bidirectional flows possibly related to the separator reconnection. While at the flare ribbons, the hot Fe XXI 1354.08 angstrom line shows blueshifts and the cool Si IV 1402.77 angstrom, C II 1335.71 angstrom, and Mg II 2803.52 angstrom lines show evident redshifts up to a velocity of 80 km s(-1), which are consistent with the scenario of chromospheric evaporation/condensation.en_US
dc.description.sponsorshipNorwegian Space Center (NSC, Norway) through an ESA PRODEX contract; NSFC 11373023 11403011 11733003 11233008 11427803; NKBRSF 2014CB744203; ASO-S grant U1731241; CAS Pioneer Hundred Talents Program;en_US
dc.rightsCC BY 3.0en_US
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/legalcodeen_US
dc.titleSpectroscopic Observations of Magnetic Reconnection and Chromospheric Evaporation in an X-shaped Solar Flareen_US
dc.typeArticleen_US
mus.citation.issue2en_US
mus.citation.journaltitleAstrophysical Journalen_US
mus.citation.volume848en_US
mus.identifier.categoryPhysics & Mathematicsen_US
mus.identifier.doi10.3847/1538-4357/aa89e4en_US
mus.relation.collegeCollege of Letters & Scienceen_US
mus.relation.departmentPhysics.en_US
mus.relation.universityMontana State University - Bozemanen_US


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