Global mantle flow and the development of seismic anisotropy: Differences between the oceanic and continental upper mantle

被引:145
作者
Conrad, Clinton P.
Behn, Mark D.
Silver, Paul G.
机构
[1] Johns Hopkins Univ, Dept Earth & Planetary Sci, Baltimore, MD 21218 USA
[2] Woods Hole Oceanog Inst, Dept Geol & Geophys, Woods Hole, MA 02543 USA
[3] Carnegie Inst Sci, Dept Terr Magnetism, Washington, DC 20015 USA
基金
美国国家科学基金会;
关键词
D O I
10.1029/2006JB004608
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
[1] Viscous shear in the asthenosphere accommodates relative motion between Earth's surface plates and underlying mantle, generating lattice-preferred orientation (LPO) in olivine aggregates and a seismically anisotropic fabric. Because this fabric develops with the evolving mantle flow field, observations of seismic anisotropy can constrain asthenospheric flow patterns if the contribution of fossil lithospheric anisotropy is small. We use global viscous mantle flow models to characterize the relationship between asthenospheric deformation and LPO and compare the predicted pattern of anisotropy to a global compilation of observed shear wave splitting measurements. For asthenosphere >500 km from plate boundaries, simple shear rotates the LPO toward the infinite strain axis (ISA, the LPO after infinite deformation) faster than the ISA changes along flow lines. Thus we expect the ISA to approximate LPO throughout most of the asthenosphere, greatly simplifying LPO predictions because strain integration along flow lines is unnecessary. Approximating LPO with the ISA and assuming A-type fabric ( olivine a axis parallel to ISA), we find that mantle flow driven by both plate motions and mantle density heterogeneity successfully predicts oceanic anisotropy (average misfit 13 degrees). Continental anisotropy is less well fit (average misfit 41 degrees), but lateral variations in lithospheric thickness improve the fit in some continental areas. This suggests that asthenospheric anisotropy contributes to shear wave splitting for both continents and oceans but is overlain by a stronger layer of lithospheric anisotropy for continents. The contribution of the oceanic lithosphere is likely smaller because it is thinner, younger, and less deformed than its continental counterpart.
引用
收藏
页数:17
相关论文
共 81 条
[11]   Convective instability of thickening mantle lithosphere [J].
Conrad, CP .
GEOPHYSICAL JOURNAL INTERNATIONAL, 2000, 143 (01) :52-70
[12]   The growth of Rayleigh-Taylor-type instabilities in the lithosphere for various rheological and density structures [J].
Conrad, CP ;
Molnar, P .
GEOPHYSICAL JOURNAL INTERNATIONAL, 1997, 129 (01) :95-112
[13]   Seismic tomography, surface uplift, and the breakup of Gondwanaland: Integrating mantle convection backwards in time [J].
Conrad, CP ;
Gurnis, M .
GEOCHEMISTRY GEOPHYSICS GEOSYSTEMS, 2003, 4
[14]   Influence of continental roots and asthenosphere on plate-mantle coupling [J].
Conrad, CP ;
Lithgow-Bertelloni, C .
GEOPHYSICAL RESEARCH LETTERS, 2006, 33 (05)
[15]   Dislocation creep in MgSiO3 perovskite at conditions of the Earth's uppermost lower mantle [J].
Cordier, P ;
Ungár, T ;
Zsoldos, L ;
Tichy, G .
NATURE, 2004, 428 (6985) :837-840
[16]   Global azimuthal seismic anisotropy and the unique plate-motion deformation of Australia [J].
Debayle, E ;
Kennett, B ;
Priestley, K .
NATURE, 2005, 433 (7025) :509-512
[17]   EFFECT OF RECENT REVISIONS TO THE GEOMAGNETIC REVERSAL TIME-SCALE ON ESTIMATES OF CURRENT PLATE MOTIONS [J].
DEMETS, C ;
GORDON, RG ;
ARGUS, DF ;
STEIN, S .
GEOPHYSICAL RESEARCH LETTERS, 1994, 21 (20) :2191-2194
[18]   RELATIVE MOTIONS BETWEEN OCEANIC PLATES OF THE PACIFIC BASIN [J].
ENGEBRETSON, DC ;
COX, A ;
GORDON, RG .
JOURNAL OF GEOPHYSICAL RESEARCH, 1984, 89 (NB12) :291-310
[19]   Shear-wave splitting beneath the Galapagos archipelago [J].
Fontaine, FR ;
Hooft, EEE ;
Burkett, PG ;
Toomey, DR ;
Solomon, SC ;
Silver, PG .
GEOPHYSICAL RESEARCH LETTERS, 2005, 32 (21) :1-4
[20]   EARLY STRUCTURAL EVOLUTION AND ANISOTROPY OF OCEANIC UPPER MANTLE [J].
FORSYTH, DW .
GEOPHYSICAL JOURNAL OF THE ROYAL ASTRONOMICAL SOCIETY, 1975, 43 (01) :103-162