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.
M., Raeder, J., and Poedts, S
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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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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.
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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.