Physics
Scientific paper
Dec 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agufmgp11a1063k&link_type=abstract
American Geophysical Union, Fall Meeting 2002, abstract #GP11A-1063
Physics
1519 Magnetic Mineralogy And Petrology, 1533 Remagnetization, 1540 Rock And Mineral Magnetism, 6030 Magnetic Fields And Magnetism, 6240 Meteorites And Tektites
Scientific paper
In early solar system history are several electromagnetic processes expected capable of magnetizing the primitive solid particles condensating from the Solar Nebula. The signature of this magnetic events can be observed in meteorites found on the Earth. It can take a long time from meteorite fall till laboratory study. Some samples are deposited in the desert or Antarctic ice for thousands of years. In this work we used the sample of the LL chondrite found in Libya desert for weathering simulations, magnetic mineralogy and magnetic properties study. The weathering in this sample is related to the desert varnish formation. From high and low temperature magnetic susceptibility measurements we can see, that most important magnetic carriers are iron, magnetite and hematite. The influence on magnetic mineralogy can be seen from weathering simulations done by leaching the samples in different solutions. This change affects the suitability of different samples for primary magnetic record study. Acknowledgements: This work is supported by Charles University Grant Agency, Czech Republic and would not be possible without the help of following people: Jakub Haloda, Petr Jakes, Marcela Bukovanska, Jaroslav Kadlec, Libuse Kohoutova, Vladimir Kohout.
Kletetschka Gunther
Kobr M.
Kohout Tomas
Pruner Petr
Wasilewski Peter J.
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