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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Systematic 3D resistive MHD simulations find that Alfvén wings narrow and close with higher stellar wind speeds, open with stronger stellar magnetic fields, and show linear scaling between magnetotail length and upstream forcing parameters.
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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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Stellar Wind Driven Alfv\'en Wing Dynamics in Planetary and Exoplanetary Magnetospheres
Systematic 3D resistive MHD simulations find that Alfvén wings narrow and close with higher stellar wind speeds, open with stronger stellar magnetic fields, and show linear scaling between magnetotail length and upstream forcing parameters.