Extreme Heating of Minor Ions in Imbalanced Solar-wind Turbulence
Minor ions in the solar corona are heated to extreme temperatures, far in excess of those of the electrons and protons that comprise the bulk of the plasma. These highly nonthermal distributions make minor ions sensitive probes of the collisionless processes that heat the corona and power the solar...
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Main Authors: | Michael F. Zhang, Matthew W. Kunz, Jonathan Squire, Kristopher G. Klein |
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Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
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Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/ad95fc |
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