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.
Living Reviews in Solar Physics , archivePrefix = "arXiv", eprint =
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Multi-technique observations constrain the configuration of the ξ Tau system, detecting orbital oscillations on multiple timescales and suggesting component C is itself a binary.
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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.
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Configuration of the $\xi$ Tau system constrained by multi-technique observations
Multi-technique observations constrain the configuration of the ξ Tau system, detecting orbital oscillations on multiple timescales and suggesting component C is itself a binary.