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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3 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 3representative citing papers
No bursty planet-induced radio emission detected from five inactive M dwarfs; upper limits constrain GJ 367 b magnetosphere to <0.8 G under assumed stellar wind conditions.
A review synthesizing manifestations of magnetic activity in cool stars and its relevance to exoplanet science via the solar-stellar connection.
citing papers explorer
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Impact Plasma Amplification of the Ancient Mercury Magnetic Field
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.