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Phase-space Energization.pdf
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Final Published Version
Author
Juno, JamesBrown, Collin R.
Howes, Gregory G.
Haggerty, Colby C.
TenBarge, Jason M.
Wilson III, Lynn B.
Caprioli, Damiano
Klein, Kristopher G.
Affiliation
Lunar and Planetary Laboratory, University of ArizonaIssue Date
2023-02-08
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American Astronomical SocietyCitation
James Juno et al 2023 ApJ 944 15Journal
The Astrophysical JournalRights
© 2023. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.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
Examining energization of kinetic plasmas in phase space is a growing topic of interest, owing to the wealth of data in phase space compared to traditional bulk energization diagnostics. Via the field-particle correlation (FPC) technique and using multiple means of numerically integrating the plasma kinetic equation, we have studied the energization of ions in phase space within oblique collisionless shocks. The perspective afforded to us with this analysis in phase space allows us to characterize distinct populations of energized ions. In particular, we focus on ions that reflect multiple times off the shock front through shock-drift acceleration, and how to distinguish these different reflected populations in phase space using the FPC technique. We further extend our analysis to simulations of three-dimensional shocks undergoing more complicated dynamics, such as shock ripple, to demonstrate the ability to recover the phase-space signatures of this energization process in a more general system. This work thus extends previous applications of the FPC technique to more realistic collisionless shock environments, providing stronger evidence of the technique's utility for simulation, laboratory, and spacecraft analysis.Note
Open access journalISSN
0004-637XEISSN
1538-4357Version
Final published versionSponsors
National Science Foundationae974a485f413a2113503eed53cd6c53
10.3847/1538-4357/acaf53
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Except where otherwise noted, this item's license is described as © 2023. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.