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    The Solar Probe Cup on the Parker Solar Probe

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    Case_2020_ApJS_246_43.pdf
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    Description:
    Final Published Version
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    Author
    Case, A. W. cc
    Kasper, Justin C.
    Stevens, Michael L.
    Korreck, Kelly E.
    Paulson, Kristoff
    Daigneau, Peter
    Caldwell, Dave
    Freeman, Mark
    Henry, Thayne
    Klingensmith, Brianna
    Bookbinder, J. A.
    Robinson, Miles
    Berg, Peter
    Tiu, Chris
    Wright, K. H.
    Reinhart, Matthew J.
    Curtis, David
    Ludlam, Michael
    Larson, Davin
    Whittlesey, Phyllis
    Livi, Roberto
    Klein, Kristopher G.
    Martinović, Mihailo M.
    Show allShow less
    Affiliation
    Univ Arizona, Lunar & Planetary Lab
    Issue Date
    2020-02-03
    Keywords
    Solar wind
    Solar instruments
    Space plasmas
    Space vehicle instruments
    Solar corona
    
    Metadata
    Show full item record
    Publisher
    IOP PUBLISHING LTD
    Citation
    A. W. Case et al 2020 ApJS 246 43
    Journal
    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
    Rights
    © 2020. The American Astronomical Society.
    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
    Solar Probe Cup (SPC) is a Faraday cup instrument on board NASA's Parker Solar Probe (PSP) spacecraft designed to make rapid measurements of thermal coronal and solar wind plasma. The spacecraft is in a heliocentric orbit that takes it closer to the Sun than any previous spacecraft, allowing measurements to be made where the coronal and solar wind plasma is being heated and accelerated. The SPC instrument was designed to be pointed directly at the Sun at all times, allowing the solar wind (which is flowing primarily radially away from the Sun) to be measured throughout the orbit. The instrument is capable of measuring solar wind ions with an energy between 100 and 6000 V (protons with speeds from 139 to 1072 km s(-1)). It also measures electrons with an energy/charge between 100 and 1500 V. SPC has been designed to have a wide dynamic range that is capable of measuring protons and alpha particles at the closest perihelion (9.86 solar radii from the center of the Sun) and out to 0.25 au. Initial observations from the first orbit of PSP indicate that the instrument is functioning well.
    ISSN
    0067-0049
    EISSN
    1538-4365
    DOI
    10.3847/1538-4365/ab5a7b
    Version
    Final published version
    ae974a485f413a2113503eed53cd6c53
    10.3847/1538-4365/ab5a7b
    Scopus Count
    Collections
    UA Faculty Publications

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