SUMMARY The velocity field is the most complete description of the active kinematics of a wide zone of active deformation. A simple method is described here for estimating the horizontal velocity field in a network of traverses that span the zone. The sum of the relative velocities in such a zone must equal the relative motion of the boundaries, which can usually be determined independently from sea-floor magnetic anomalies. Also, if traverses intersect each other, the velocity of the point of intersection relative to one of the boundaries of the zone, must be the same regardless of the traverse segment along which relative velocities have been summed. In addition, rates of deformation within parts of the deforming zone can be estimated from field observations. All these constraints can be expressed as linear equations. The aim is to maximize the difference between the number of equations (N) and unknowns (M), with the formed exceeding the latter. The problem can be expressed in matrix form: Am = d, where A is an N X M model matrix of constraints, d is a column vector of data, and m is the solution vector of unknowns. If N > M, a solution for m can be determined by minimizing a function of I(Am - dll, using standard techniques and taking into account any uncertainty in the data vector d. This method is used to estimate the velocity field in the Californian plate-boundary zone. A weighted least-squares solution is found that predicts tectonic rotations. Simple tests illustrate the effect on the derived velocity field of changing features of the velocity model.
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