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Influences of lower-mantle properties on the formation of asthenosphere in oceanic upper mantle

Yuen, D.A. and Tosi, Nicola and Cadek, O. (2011) Influences of lower-mantle properties on the formation of asthenosphere in oceanic upper mantle. Journal of Earth Science, 22 (2), pp. 143-154. Springer. doi: 10.1007/s12583-011-0166-9.

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Official URL: http://www.springerlink.com/content/rgjq157jk61n6172/


Asthenosphere is a venerable concept based on geological intuition of Reginald Daly nearly 100 years ago. There have been various explanations for the existence of the asthenosphere. The concept of a plume-fed asthenosphere has been around for a few years due to the ideas put forth by Yamamoto et al.. Using a two-dimensional Cartesian code based on finite-volume method, we have investigated the influences of lower-mantle physical properties on the formation of a low-viscosity zone in the oceanic upper mantle in regions close to a large mantle upwelling. The rheological law is Newtonian and depends on both temperature and depth. An extended-Boussinesq model is assumed for the energetics and the olivine to spinel, the spinel to perovskite and perovskite to post-perovskite (ppv) phase transitions are considered. We have compared the differences in the behavior of hot upwellings passing through the transition zone in the mid-mantle for a variety of models, starting with constant physical properties in the lower-mantle and culminating with complex models which have the post-perovskite phase transition and depth-dependent coefficient of thermal expansion and thermal conductivity. We found that the formation of the asthenosphere in the upper mantle in the vicinity of large upwellings is facilitated in models where both depth-dependent thermal expansivity and conductivity are included. Models with constant thermal expansivity and thermal conductivity do not produce a hot low-viscosity zone, resembling the asthenosphere. We have also studied the influences of a cylindrical model and found similar results as the Cartesian model with the important difference that upper-mantle temperatures were much cooler than the Cartesian model by about 600 to 700 K. Our findings argue for the potentially important role played by lower-mantle material properties on the development of a plume-fed asthenosphere in the oceanic upper mantle.

Item URL in elib:https://elib.dlr.de/60141/
Document Type:Article
Title:Influences of lower-mantle properties on the formation of asthenosphere in oceanic upper mantle
AuthorsInstitution or Email of AuthorsAuthor's ORCID iD
Yuen, D.A.University of Minnesota, Minneapolis, MN, USAUNSPECIFIED
Tosi, Nicolanicola.tosi (at) dlr.deUNSPECIFIED
Cadek, O.Charles University in Prague, Prague, Czech RepublicUNSPECIFIED
Journal or Publication Title:Journal of Earth Science
Refereed publication:Yes
Open Access:No
Gold Open Access:No
In ISI Web of Science:Yes
DOI :10.1007/s12583-011-0166-9
Page Range:pp. 143-154
Keywords:oceanic asthenosphere, lower mantle, thermal expansivity, thermal conductivity, phase transition
HGF - Research field:Aeronautics, Space and Transport (old)
HGF - Program:Space (old)
HGF - Program Themes:W EW - Erforschung des Weltraums
DLR - Research area:Space
DLR - Program:W EW - Erforschung des Weltraums
DLR - Research theme (Project):W - Vorhaben Exploration des Sonnensystems (old)
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Planetary Physics
Institute of Planetary Research
Deposited By: Noack, Lena
Deposited On:28 Sep 2011 14:55
Last Modified:01 Dec 2018 19:46

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