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.
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MMS observations show distinct electron populations inside a magnetic cloud, on Alfvén wing field lines, and on closed lines, including signatures of dual wing reconnection during a 2023 CME.
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MMS Insights into CME Driven Sub-Alfv\'enic Solar Wind at 1 AU
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.
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Earth's Alfv\'{e}n Wings: Unveiling Dynamic Variations of Field-line Topologies with Electron Distributions
MMS observations show distinct electron populations inside a magnetic cloud, on Alfvén wing field lines, and on closed lines, including signatures of dual wing reconnection during a 2023 CME.