The lateral variation of P n velocity gradient under Eurasia

Mantle lid P wave velocity gradient, or P n velocity gradient, reflects the depth and lateral variations of thermal and rheological state of the uppermost mantle. Mapping the P n velocity gradient and its lateral variation helps us gain insight into the temperature, composition, and dynamics of the uppermost mantle. In addition, because P n velocity gradient has profound influence on P n propagation behavior, an accurate mapping of P n velocity gradient also improves the modeling and prediction of P n travel times and amplitudes. In this study, I used measured P n travel times to derive path‐specific P n velocity gradients. I then inverted these velocity gradients for two‐dimensional (2‐D) P n velocity‐gradient models for Eurasia based on the assumption that a path‐specific P n velocity gradient is the mean of laterally varying P n velocity gradients along the P n path. Result from a Monte Carlo simulation indicates that the assumption is appropriate. The 2‐D velocity‐gradient models show that most of Eurasia has positive velocity gradients. High velocity gradients exist mainly in tectonically active regions. Most tectonically stable regions show low and more uniform velocity gradients. Strong velocity‐gradient variations occur largely along convergent plate boundaries, particularly under overriding plates.