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dc.contributor.authorNeugebauer, M.
dc.contributor.authorSterling, A.C.
dc.date.accessioned2021-11-29T20:24:35Z
dc.date.available2021-11-29T20:24:35Z
dc.date.issued2021
dc.identifier.citationNeugebauer, M., & Sterling, A. C. (2021). Relation of Microstreams in the Polar Solar Wind to Switchbacks and Coronal X-Ray Jets. Astrophysical Journal Letters.
dc.identifier.issn2041-8205
dc.identifier.doi10.3847/2041-8213/ac2945
dc.identifier.urihttp://hdl.handle.net/10150/662372
dc.description.abstractUlysses data obtained at high solar latitudes during periods of minimum solar activity in 1994 and 2007 are examined to determine the relation between velocity structures called microstreams and folds in the magnetic field called switchbacks. A high correlation is found. The possibility of velocity peaks in microstreams originating from coronal X-ray jets is reexamined; we now suggest that microstreams are the consequence of the alternation of patches of switchbacks and quiet periods, where the switchbacks could be generated by minifilament/flux rope eruptions that cause coronal jets. © 2021. The American Astronomical Society. All rights reserved.
dc.language.isoen
dc.publisherAmerican Astronomical Society
dc.rightsCopyright © 2021. The American Astronomical Society. All rights reserved.
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.titleRelation of Microstreams in the Polar Solar Wind to Switchbacks and Coronal X-Ray Jets
dc.typeArticle
dc.typetext
dc.contributor.departmentLunar and Planetary Laboratory, University of Arizona
dc.identifier.journalAstrophysical Journal Letters
dc.description.noteImmediate access
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
dc.eprint.versionFinal published version
dc.source.journaltitleAstrophysical Journal Letters
refterms.dateFOA2021-11-29T20:24:35Z


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