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Cosmic-Ray-Produced Noble Gases in Meteorites

2002; Mineralogical Society of America; Volume: 47; Issue: 1 Linguagem: Inglês

10.2138/rmg.2002.47.5

1943-2666

R. Wieler,

Geology and Paleoclimatology Research

Research Article| January 01, 2002 Cosmic-Ray-Produced Noble Gases in Meteorites Rainer Wieler Rainer Wieler Isotope Geology, ETH-Zürich, Sonneggstrasse 5, CH-8092 Zürich, Switzerland, wieler@2erdw.ethz.ch Search for other works by this author on: GSW Google Scholar Author and Article Information Rainer Wieler Isotope Geology, ETH-Zürich, Sonneggstrasse 5, CH-8092 Zürich, Switzerland, wieler@2erdw.ethz.ch Publisher: Mineralogical Society of America First Online: 13 Jul 2017 © The Mineralogical Society Of America Reviews in Mineralogy and Geochemistry (2002) 47 (1): 125–170. https://doi.org/10.2138/rmg.2002.47.5 Article history First Online: 13 Jul 2017 Cite View This Citation Add to Citation Manager Share Icon Share Facebook Twitter LinkedIn Email Permissions Search Site Citation Rainer Wieler; Cosmic-Ray-Produced Noble Gases in Meteorites. Reviews in Mineralogy and Geochemistry 2002;; 47 (1): 125–170. doi: https://doi.org/10.2138/rmg.2002.47.5 Download citation file: Ris (Zotero) Refmanager EasyBib Bookends Mendeley Papers EndNote RefWorks BibTex toolbar search Search Dropdown Menu toolbar search search input Search input auto suggest filter your search All ContentBy SocietyReviews in Mineralogy and Geochemistry Search Advanced Search Energetic particles of the galactic cosmic radiation (GCR) have a mean penetration depth in rock of about 50 cm, comparable to the typical size of a meteorite. GCR-induced effects therefore provide a means to study the history of meteorites as small objects in space or in the top few meters of their parent body. These effects include cosmic ray tracks, i.e., the radiation damage trails in a crystal lattice produced by heavy ions in the GCR (Fleischer et al. 1975), and thermoluminescence, i.e., the light emitted by a heated sample which had been irradiated by energetic particles (... You do not have access to this content, please speak to your institutional administrator if you feel you should have access.