Abstract
We employ a new thermodynamic method for self-consistent computation of compositional and thermal effects on phase transition depths, density, and seismic velocities. Using these profi les, we compare theoretical and observed differential traveltimes between P410s and P (T 410 ) and between P600s and P410s (T 660‐410 ) that are affected only by seismic structure in the upper mantle. The anticorrelation between T 410 and T 660‐410 suggests that variations in T 410 and T 660‐410 of ~8 s are due to lateral temperature variations in the upper mantle transition zone of ~400 K. If the mantle is a mechanical mixture of basaltic and harzburgitic components, our traveltime data suggest that the mantle has an average temperature of 1600 ± 50 K, in agreement with temperature estimates from magma compositions of mid-ocean ridge basalts. We infer a 100 K hotter mantle if we assume the mantle to have a homogeneous pyrolitic composition. The transition-zone temperature beneath hotspots and within subduction zones is relatively high and low, respectively. However, the largest variability in T 410 and T 660‐410 is recorded by global stations far from subduction zones and hotspots. This indicates that the 400 K variation in upper mantle temperature is complicated by tilted upwellings, slab fl attening and accumulation, ancient subduction, and processes unrelated to present-day subduction and plume ascent.
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