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Cosmogenic neon from individual grains of CM meteorites - Extremely long pre-compaction exposure histories or an enhanced early particle fluxThis paper presents the results on cosmogenic Ne extracted from individual meteoritic grains by a laser extraction system which used, at different times, two CW lasers: an Ar-ion laser and an Nd:YAG laser, with 20 and 70 W of deliverable power, respectively. Chemical etching was used to select grains exposed to solar flare VH particles. Results show that most of the grains with solar flare VH tracks (but not those which did not exhibit such tracks) contain spallation-produed Ne in significant excess of that due to the nominal cosmic-ray exposure, providing evidence for extensive energetic particle exposure during the precompaction era.
Document ID
19900056743
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Hohenberg, Charles M.
(Washington Univ. Technology Associates, Inc. Saint Louis, MO, United States)
Nichols, Robert H., Jr.
(Washington Univ. Technology Associates, Inc. Saint Louis, MO, United States)
Olinger, Chad T.
(Washington University Saint Louis, MO, United States)
Goswami, J. N.
(Physical Research Laboratory Ahmedabad, India)
Date Acquired
August 14, 2013
Publication Date
July 1, 1990
Publication Information
Publication: Geochimica et Cosmochimica Acta
Volume: 54
ISSN: 0016-7037
Subject Category
Lunar And Planetary Exploration
Accession Number
90A43798
Funding Number(s)
CONTRACT_GRANT: NAG9-7
CONTRACT_GRANT: NGT-50194
Distribution Limits
Public
Copyright
Other

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