Magnification of pre-existing magnetic fields in impact-produced plasmas, with reference to impact craters

Statistics – Computation

Scientific paper

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Geomagnetism, Hypervelocity Impact, Impact Damage, Planetary Magnetic Fields, Plasma Clouds, Basalt, Cratering, Plasma Density, Plasma Temperature

Scientific paper

It is proposed that the strong temperature and density gradients at the boundary of an impact-produced plasma cloud may be a source of local magnetic field amplification. The plasma produced by the 10 km/sec impact of an aluminum projectile on basalt yields a magnetic field through thermally-driven electrical currents which can account for the magnetic profile exhibited by impacted samples. Although the computations presented refer to a particular, experimental situation, the mechanism proposed may be more generally applicable to planetary cratering and account for the magnetization observed in the vicinity of lunar craters. Such studies as Martelli and Newton (1977) confirm the magnetic field enhancement near the crater edges.

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