Figure 10.
Stability of Euler pole estimates as a function of ISC model exploration. (a) χ2 as a function of the imposed σm constraints for the dip-slip component with a priori model m0 = 0, Dc = 30 km and fixed regularization parameters for the strike-slip component. Blue square is the best model for an ISC model with σm = 20 mm yr−1. (b) Predicted velocity magnitude at several sites within the North Andean West (NAW) block using Euler pole estimates for ISC models with σm values of 8, 20 and 35 mm yr−1. Predicted velocities range from 76.2°W at latitude 2.3°S to 76.6°W at latitude 6°N. (c) Same as (b) but for predicted velocity azimuths.

Stability of Euler pole estimates as a function of ISC model exploration. (a) χ2 as a function of the imposed σm constraints for the dip-slip component with a priori model m0 = 0, Dc = 30 km and fixed regularization parameters for the strike-slip component. Blue square is the best model for an ISC model with σm = 20 mm yr−1. (b) Predicted velocity magnitude at several sites within the North Andean West (NAW) block using Euler pole estimates for ISC models with σm values of 8, 20 and 35 mm yr−1. Predicted velocities range from 76.2°W at latitude 2.3°S to 76.6°W at latitude 6°N. (c) Same as (b) but for predicted velocity azimuths.

Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close