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 reveal a knotted, non-coplanar electron diffusion region in Earth's magnetotail reconnection where the EDR plane deviates 38 degrees from the IDR, the guide field rotates and strengthens, and Hall magnetic fields differ in structure between electron and ion scales.
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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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Observation of a Knotted Electron Diffusion Region in Earth's Magnetotail Reconnection
MMS observations reveal a knotted, non-coplanar electron diffusion region in Earth's magnetotail reconnection where the EDR plane deviates 38 degrees from the IDR, the guide field rotates and strengthens, and Hall magnetic fields differ in structure between electron and ion scales.