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MASS-TRANSFER OF HELIUM, NEON, ARGON, AND XENON THROUGH A STEADY-STATE UPPER-MANTLE

Abstract:

We have examined the steady-state upper mantle model for helium, neon, argon, and xenon following the mass transfer approach presented by Kellogg and Wasserburg (1990) for helium and Porcelli and Wasserburg (1995a) for xenon. The model explains the available observational data of mantle helium, neon, argon, and xenon isotope compositions and provides specific predictions regarding the rare gas isotopic compositions of the lower mantle, subduction of rare gases, and mantle rare gas concentrati...

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Publication status:
Published

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Institution:
University of Oxford
Division:
MPLS
Department:
Earth Sciences
Role:
Author
Journal:
GEOCHIMICA ET COSMOCHIMICA ACTA More from this journal
Volume:
59
Issue:
23
Pages:
4921-4937
Publication date:
1995-12-01
DOI:
ISSN:
0016-7037
Pubs id:
pubs:165154
UUID:
uuid:69f39849-924b-41ab-88fe-1bacffd42773
Local pid:
pubs:165154
Source identifiers:
165154
Deposit date:
2012-12-19

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