Mantle 3He distribution and deep circulation in the Indian Ocean
Mantle 3He distribution and deep circulation in the Indian Ocean
Date
2004-06-10
Authors
Srinivasan, Ashwanth
Top, Zafer
Schlosser, Peter
Hohmann, Roland
Iskandarani, Mohamed
Olson, Donald B.
Lupton, John E.
Jenkins, William J.
Top, Zafer
Schlosser, Peter
Hohmann, Roland
Iskandarani, Mohamed
Olson, Donald B.
Lupton, John E.
Jenkins, William J.
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DOI
10.1029/2003JC002028
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Keywords
Indian Ocean
Tracers
Deep circulation
Tracers
Deep circulation
Abstract
The World Ocean Circulation Experiment Indian Ocean helium isotope data are mapped and features of intermediate and deep circulation are inferred and discussed. The 3He added to the deep Indian Ocean originates from (1) a strong source on the mid-ocean ridge at about 19°S/65°E, (2) a source located in the Gulf of Aden in the northwestern Indian Ocean, (3) sources located in the convergent margins in the northeastern Indian Ocean, and (4) water imported from the Indonesian Seas. The main circulation features inferred from the 3He distribution include (1) deep (2000–3000 m) eastward flow in the central Indian Ocean, which overflows into the West Australian Basin through saddles in the Ninetyeast Ridge, (2) a deep (2000–3000 m) southwestward flow in the western Indian Ocean, and (3) influx of Banda Sea Intermediate Waters associated with the deep core (1000–1500 m) of the through flow from the Pacific Ocean. The large-scale 3He distribution is consonant with the known pathways of deep and bottom water circulation in the Indian Ocean.
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Author Posting. © American Geophysical Union, 2004. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Journal of Geophysical Research 109 (2004): C06012, doi:10.1029/2003JC002028.
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Journal of Geophysical Research 109 (2004): C06012