Some block motions are well defined and vary little within our model. The Eurasian block, Australian block, and Indian block rotation parameters are defined primarily by
the sites that lie within the stable interior and are affected very little by plate boundary strain. With respect to Eurasia the pole of rotation for the Indian plate is
located at 23.6410.979N 8.7324.402E with an angular rotation rate of 0.3590.012 Myr-1 (Figure 2.43). Relative poles
shown in Figure 2.43 illustrate the consistency of our solution.
Along the Himalayan Range Front we estimate IND-EUR convergence to vary from 34-41 mm/yr from 76 -91 east longitude (Figure 2.44,
inset). We parameterize the Himalayan front with four main blocks defined by the major geologic features like the Indus-Zangbo suture, Gulu rift, and Karakorum fault. As
much as 25 mm/yr of contraction is accommodated by the Himalayan thrust (Figure 2.44). Our model, along the front, fit the data quite well. Some systematic
misfit with the Himalayan blocks may be related to unmodeled east-west extension.
Relative plate poles of India's motion with respect to Eurasia. Values that precede the reference are the poles' magnitude
measured in deg/My with a counter-clockwise positive convention.
Velocity profile of measured and predicted velocities in Tibet. The inset figure shows the block configuration used in the
inversion. GPS stations are colored according to source.
Berkeley Seismological Laboratory
215 McCone Hall, UC Berkeley, Berkeley, CA 94720-4760
Questions or comments? Send e-mail: firstname.lastname@example.org
© 2007, The Regents of the University of California