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arxiv: 2402.08091 · v4 · pith:3RWD6AW3new · submitted 2024-02-12 · ⚛️ physics.space-ph · astro-ph.EP· astro-ph.SR

Earth's Alfv\'en wings driven by the April 2023 Coronal Mass Ejection

classification ⚛️ physics.space-ph astro-ph.EPastro-ph.SR
keywords magnetospherealfvearthplasmaaprilcoldcoronalejection
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We report a rare regime of Earth's magnetosphere interaction with sub-Alfv\'enic solar wind in which the windsock-like magnetosphere transforms into one with Alfv\'en wings. In the magnetic cloud of a Coronal Mass Ejection (CME) on April 24, 2023, NASA's Magnetospheric Multiscale mission distinguishes the following features: (1) unshocked and accelerated cold CME plasma coming directly against Earth's dayside magnetosphere; (2) dynamical wing filaments representing new channels of magnetic connection between the magnetosphere and foot points of the Sun's erupted flux rope; (3) cold CME ions observed with energized counter-streaming electrons, evidence of CME plasma captured due to reconnection between magnetic-cloud and Alfv\'en-wing field lines. The reported measurements advance our knowledge of CME interaction with planetary magnetospheres, and open new opportunities to understand how sub-Alfv\'enic plasma flows impact astrophysical bodies such as Mercury, moons of Jupiter, and exoplanets close to their host stars.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Earth's Alfv\'{e}n Wings: Unveiling Dynamic Variations of Field-line Topologies with Electron Distributions

    physics.space-ph 2024-08 unverdicted novelty 6.0

    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.