Savani: A variable resolution whole-mantle model of anisotropic shear velocity variations based on multiple data sets

被引:206
作者
Auer, L. [1 ]
Boschi, L. [2 ,3 ]
Becker, T. W. [4 ]
Nissen-Meyer, T. [5 ]
Giardini, D. [1 ]
机构
[1] ETH, Inst Geophys, CH-8093 Zurich, Switzerland
[2] Univ Paris 06, Sorbonne Univ, Inst Sci Terre Paris ISTeP, Paris, France
[3] Inst Sci Terre Paris ISTeP, CNRS, Paris, France
[4] Univ So Calif, Dept Earth Sci, Los Angeles, CA USA
[5] Univ Oxford, Dept Earth Sci, Oxford OX1 3PR, England
关键词
SURFACE-WAVE TOMOGRAPHY; SEISMIC ANISOTROPY; CRUSTAL CORRECTIONS; FORM TOMOGRAPHY; TRAVEL-TIMES; BENEATH; LOVE; FLOW; DISPERSION; EVOLUTION;
D O I
10.1002/2013JB010773
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
We present a tomographic model of radially anisotropic shear velocity variations in the Earth's mantle based on a new compilation of previously published data sets and a variable block parameterization, adapted to local raypath density. We employ ray-theoretical sensitivity functions to relate surface wave and body wave data with radially anisotropic velocity perturbations. Our database includes surface wave phase delays from fundamental modes up to the sixth overtone, measured at periods between 25 and 350 s, as well as cross-correlation traveltimes of major body wave phases. Before inversion, we apply crustal corrections using the crustal model CRUST2.0, and we account for azimuthal anisotropy in the upper mantle using ray-theoretical corrections based on a global model of azimuthal anisotropy. While being well correlated with earlier models at long spatial wavelength, our preferred solution, savani, additionally delineates a number of previously unidentified structures due to its improved resolution in areas of dense coverage. This is because the density of the inverse grid ranges between 1.25 degrees in well-sampled and 5 degrees in poorly sampled regions, allowing us to resolve regional structure better than it is typically the case in global S wave tomography. Our model highlights (i) a distinct ocean-continent anisotropic signature in the uppermost mantle, (ii) an oceanic peak in above average xi<1 which is shallower than in previous models and thus in better agreement with estimates of lithosphere thickness, and (iii) a long-wavelength pattern of xi<1 associated with the large low-shear velocity provinces in the lowermost mantle.
引用
收藏
页码:3006 / 3034
页数:29
相关论文
共 89 条
[1]   UPPER MANTLE ANISOTROPY - EVIDENCE FROM FREE OSCILLATIONS [J].
ANDERSON, DL ;
DZIEWONSKI, AM .
GEOPHYSICAL JOURNAL OF THE ROYAL ASTRONOMICAL SOCIETY, 1982, 69 (02) :383-404
[2]  
Anderson O., 1995, AGU HDB, V2, P64, DOI DOI 10.1029/RF002P0064
[3]  
Babuska V., 1991, SEISMIC ANISOTROPY E
[4]  
Bassin C., 2000, Eos, V81
[5]   Radial seismic anisotropy as a constraint for upper mantle rheology [J].
Becker, Thorsten W. ;
Kustowski, Bogdan ;
Ekstrom, Goran .
EARTH AND PLANETARY SCIENCE LETTERS, 2008, 267 (1-2) :213-227
[6]   Stochastic analysis of shear-wave splitting length scales [J].
Becker, Thorsten W. ;
Browaeys, Jules T. ;
Jordan, Thomas H. .
EARTH AND PLANETARY SCIENCE LETTERS, 2007, 259 (3-4) :526-540
[7]   Statistical properties of seismic anisotropy predicted by upper mantle geodynamic models [J].
Becker, Thorsten W. ;
Chevrot, Sebastien ;
Schulte-Pelkum, Vera ;
Blackman, Donna K. .
JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH, 2006, 111 (B8)
[8]   A comparison of tomographic and geodynamic mantle models [J].
Becker, TW ;
Boschi, L .
GEOCHEMISTRY GEOPHYSICS GEOSYSTEMS, 2002, 3 :1-48
[9]  
Beghein C., 2004, GEOPH RES ABSTR, V6, P1348
[10]   Implications of grain size evolution on the seismic structure of the oceanic upper mantle [J].
Behn, Mark D. ;
Hirth, Greg ;
Elsenbeck, James R., II .
EARTH AND PLANETARY SCIENCE LETTERS, 2009, 282 (1-4) :178-189