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The left column shows the evolution of the (log-scale) plasma mass density, ๐œŒ, with velocity flow direction (white arrows)

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astro-ph.EP 1

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2025 1

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UNVERDICTED 1

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Impact Plasma Amplification of the Ancient Mercury Magnetic Field

astro-ph.EP ยท 2025-10-02 ยท unverdicted ยท novelty 6.0

Impact plasma from a Caloris-size basin formation amplifies Mercury's ancient magnetospheric field from 0.5-0.9 uT to ~13 uT, recording SRM that yields ~5 nT crustal fields at 20 km altitude antipodal to the basin.

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  • Impact Plasma Amplification of the Ancient Mercury Magnetic Field astro-ph.EP ยท 2025-10-02 ยท unverdicted ยท none ยท ref 24

    Impact plasma from a Caloris-size basin formation amplifies Mercury's ancient magnetospheric field from 0.5-0.9 uT to ~13 uT, recording SRM that yields ~5 nT crustal fields at 20 km altitude antipodal to the basin.