TY - JOUR
T1 - Lateral variations in upper mantle thermal structure inferred from three‐dimensional seismic inversion models
AU - Yan, Ben
AU - Graham, E. K.
AU - Furlong, K. P.
PY - 1989/5
Y1 - 1989/5
N2 - Global shear wave velocity variations in the upper mantle (Woodhouse and Dziewonski, 1984) are employed as a basis for inferring lateral heterogeneities in temperature or composition at a depth of 150 km. Using experimentally determined elastic moduli for the olivine solid solution and Hashin‐Shtrikman bound theory, Vs and its partial derivatives with respect to temperature or composition (iron content) are calculated for the depth of interest. Based on these results, the observed seismic Vs variations are interpreted as temperature and compositional deviations relative to a spherically symmetric reference model. If it is assumed that the Vs variations primarily represent lateral temperature changes, then the present results can be used to construct a global surface heat flow map from the geotherm families of Pollack and Chapman (1977). Our inferred heat flow patterns, calculated independently of actual heat flow data, show clear agreement with the surface heat flow maps proposed by Chapman and Pollack (1975) and Chapman (1985). This result is consistent with and supports thermal structure as the primary governing factor in the generation of upper mantle lateral velocity variations. Compositional changes appear to correlate with temperature, but affect velocity structure to a lesser extent.
AB - Global shear wave velocity variations in the upper mantle (Woodhouse and Dziewonski, 1984) are employed as a basis for inferring lateral heterogeneities in temperature or composition at a depth of 150 km. Using experimentally determined elastic moduli for the olivine solid solution and Hashin‐Shtrikman bound theory, Vs and its partial derivatives with respect to temperature or composition (iron content) are calculated for the depth of interest. Based on these results, the observed seismic Vs variations are interpreted as temperature and compositional deviations relative to a spherically symmetric reference model. If it is assumed that the Vs variations primarily represent lateral temperature changes, then the present results can be used to construct a global surface heat flow map from the geotherm families of Pollack and Chapman (1977). Our inferred heat flow patterns, calculated independently of actual heat flow data, show clear agreement with the surface heat flow maps proposed by Chapman and Pollack (1975) and Chapman (1985). This result is consistent with and supports thermal structure as the primary governing factor in the generation of upper mantle lateral velocity variations. Compositional changes appear to correlate with temperature, but affect velocity structure to a lesser extent.
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U2 - 10.1029/GL016i005p00449
DO - 10.1029/GL016i005p00449
M3 - Article
AN - SCOPUS:0024484139
SN - 0094-8276
VL - 16
SP - 449
EP - 452
JO - Geophysical Research Letters
JF - Geophysical Research Letters
IS - 5
ER -