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Large-scale Structure and Turbulence Transport in the Inner Solar Wind: Comparison of Parker Solar Probe’s First Five Orbits with a Global 3D Reynolds-averaged MHD Model

Crossref DOI link: https://doi.org/10.3847/1538-4357/ac1ac7

Published Online: 2021-12-14

Published Print: 2021-12-01

Update policy: https://doi.org/10.1088/crossmark-policy

Authors

Chhiber, Rohit https://orcid.org/0000-0002-7174-6948
Usmanov, Arcadi V. https://orcid.org/0000-0002-0209-152X
Matthaeus, William H. https://orcid.org/0000-0001-7224-6024
Goldstein, Melvyn L. https://orcid.org/0000-0002-5317-988X
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Article Title: Large-scale Structure and Turbulence Transport in the Inner Solar Wind: Comparison of Parker Solar Probe’s First Five Orbits with a Global 3D Reynolds-averaged MHD Model

Journal Title: The Astrophysical Journal

Article Type: paper

Copyright Information: © 2021. The American Astronomical Society. All rights reserved.

Publication dates

Date Received: 2021-05-22

Date Accepted: 2021-08-03

Online publication date: 2021-12-14

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