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    Relation of Microstreams in the Polar Solar Wind to Switchbacks and Coronal X-Ray Jets

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    Neugebauer_2021_ApJL_920_L31.pdf
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    Author
    Neugebauer, M.
    Sterling, A.C.
    Affiliation
    Lunar and Planetary Laboratory, University of Arizona
    Issue Date
    2021
    
    Metadata
    Show full item record
    Publisher
    American Astronomical Society
    Citation
    Neugebauer, M., & Sterling, A. C. (2021). Relation of Microstreams in the Polar Solar Wind to Switchbacks and Coronal X-Ray Jets. Astrophysical Journal Letters.
    Journal
    Astrophysical Journal Letters
    Rights
    Copyright © 2021. The American Astronomical Society. All rights reserved.
    Collection Information
    This 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.
    Abstract
    Ulysses 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.
    Note
    Immediate access
    ISSN
    2041-8205
    DOI
    10.3847/2041-8213/ac2945
    Version
    Final published version
    ae974a485f413a2113503eed53cd6c53
    10.3847/2041-8213/ac2945
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    UA Faculty Publications

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