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#). The magnetized material is derived to represent a cylindrical disk volume with a 20-km radius and ranging thicknesses (Caciagli et al., 2018). The ๐œ’%

manuscript submitted to JGR: Planets Figure 13: Shock remanent magnetization efficiency, paleointensity, layer thickness of magnetized materials that can produce 5 nT crustal anomalies · 2018

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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 29

    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.