MMS data from a 2023 CME show elevated electron temperatures with superthermal tails, depleted mid-energy electrons, and weak MHD-like turbulence with reduced intermittency in the rare sub-Alfvénic solar wind at 1 AU.
S., Forman, M., & Oughton, S
2 Pith papers cite this work. Polarity classification is still indexing.
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