Magnetic classification of stony meteorites: 1. Ordinary chondrites

By P. Rochette, L. Sagnotti, M. Bourot-Denise, G. Consolmagno, L. Folco, J. Gattacceca, M. Osete, L. Pesonen. 2003

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Paleomagnetic Records of Meteorites and Early Planetesimal Differentiation (2010, background): “On the other hand, for shock pressures above ∼40 GPa, the shock-induced temperature increase (Bischoff and Stoffler 1992; Artemieva and Ivanov 2004) is usually high enough to impart a thermoremanent magnetization (TRM) to the rock during slow cooling from postshock temperatures of ∼400–1100°C.”
The significance of meteorite density and porosity (2008, background): “Unlike traditional chemical tests, the measurement of physical properties is fast and non-destructive, and it characterizes the whole rock, making it especially appropriate for surveying large collections and in detecting misidentified samples (Rochette et al., 2003).”