Physics
Scientific paper
Mar 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991metic..26....1c&link_type=abstract
Meteoritics (ISSN 0026-1114), vol. 26, March 1991, p. 1-10.
Physics
11
Achondrites, Magnetic Properties, Magnetization, Remanence, Siderites, Stony-Iron Meteorites, Demagnetization, Geomagnetism, Kamacite, Lunar Magnetic Fields, Magnetic Permeability, Solar Corona, Thermomagnetic Effects, Meteorites, Magnetic Properties, Estherville, Mesosiderites, Kamacite, Magnetic Field, Samples, Meteorite, Stony-Iron Meteorites, Tetrataenite, Remanent Magnetization, Matrix, Temperature, Magnetization, Fragments, Demagnetization, Metal, Thermal Effects, Iron Nickel, Intensity, Nrm, Origin,
Scientific paper
Taking advantage of the natural remanent magnetization (NRM) left in meteorites by the conjunction of their evolutionary processes and the effects of early solar system magnetic fields, the Estherville mesosiderite has been studied with a view to the extent to which uncertainties associated with mesosiderite history and evolution can be resolved by magnetic properties. The noncoherent directions of NRM within the matrix imply the acquisition of an initial NRM by kamacite in the fragments prior to their final accumulation into the mesosiderite material, and the presence of an ambient magnetic field when the fragment material cooled after its formation. Susceptibility anisotropy observations imply anisotropic property acquisition before final meteorite accumulation.
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