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.
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.
MMS observations document turbulence spectra and electron-scale reconnection signatures inside Kelvin-Helmholtz waves during a geomagnetic storm.
citing papers explorer
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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.
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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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Turbulence properties and kinetic signatures of electron in Kelvin-Helmholtz waves during a geomagnetic storm
MMS observations document turbulence spectra and electron-scale reconnection signatures inside Kelvin-Helmholtz waves during a geomagnetic storm.