On the use of a nuclear microprobe for trace element analysis in meteorites and cosmic dust

Details On the use of a nuclear microprobe for trace element analysis in meteorites and cosmic dust On the use of a nuclear microprobe for trace element analysis in meteorites and cosmic dust

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987nimpb..22..380v&link_type=abstract

Nuclear Instruments and Methods in Physics Research Section B, Volume 22, Issue 1-3, p. 380-385.

Physics

7

Scientific paper

Our knowledge of the chemical, physical and nuclear processes which occurred during the early history of our solar system is, besides on observations of the sun, stars and perhaps galaxies, based on laboratory studies of terrestrial, lunar and meteoritic samples. Since among these, meteorites and especially carbonaceous chondrites have been left relatively unchanged since their formation, these samples have yielded the most information. For these laboratory studies a variety of techniques has been used. This paper describes the use of a nuclear microprobe to contribute to these studies.
Permanent address: Rice University, Department of Geology, Houston, USA.

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