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MMS Observations of Energized He+ Pickup Ions at Quasiperpendicular ShocksAccelerated He+ PUIs, downstream of quasi-perpendicular shocks, are studied as 10a function of the fast mode Mach number (Mf) and shock obliquity (𝜃Bn).We analyze quasi-perpendicular shocks with Mach numbers in the range [1, 7] observed by the Magnetospheric MultiScale (MMS) mission, and compare upstream and downstream He+ velocity distribution functions (VDFs). For each shock event, we characterize the upstream PUI distribution and derive reduced 1D velocity distributions for the selected upstream and downstream intervals. We also compare the upstream to downstream ratio of spectral indices, computed from the He+ perpendicular distributions, to Mf and 𝜃Bn. We find a positive correlation between this spectral index ratio and Mf, which suggests that perpendicular energization of He+ PUIs is enhanced as the shock becomes stronger. These results inform modeling efforts of PUIs and shock acceleration processes, particularly those taking place at the termination shock.
Document ID
20210013422
Acquisition Source
Goddard Space Flight Center
Document Type
Accepted Manuscript (Version with final changes)
Authors
Michael J. Starkey ORCID
(The University of Texas at San Antonio San Antonio, Texas, United States)
S A Fuselier ORCID
(Southwest Research Institute San Antonio, Texas, United States)
M I Desai ORCID
(Southwest Research Institute San Antonio, Texas, United States)
S J Schwartz ORCID
(Laboratory for Atmospheric and Space Physics Boulder, Colorado, United States)
C. T. Russell ORCID
(University of California, Los Angeles Los Angeles, California, United States)
H. Wei ORCID
(University of California, Los Angeles Los Angeles, California, United States)
H. Madanian ORCID
(Southwest Research Institute San Antonio, Texas, United States)
J Mukherjee
(Southwest Research Institute Boulder, CO, United States)
L B Wilson III ORCID
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Date Acquired
April 9, 2021
Publication Date
May 20, 2021
Publication Information
Publication: The Astrophysical Journal
Publisher: IOP Publishing
Volume: 913
Issue: 2
Issue Publication Date: June 1, 2021
ISSN: 0004-637X
e-ISSN: 1538-4357
URL: https://iopscience.iop.org/article/10.3847/1538-4357/abf4d9
Subject Category
Astrophysics
Funding Number(s)
WBS: 958044.04.01
CONTRACT_GRANT: HQ-SG-FSP
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
Technical Review
External Peer Committee
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