Abstract
In planetary rovers a three-dimensional representation of the scene has to be obtained on the knowledge of its stereoscopic image without measuring the distance to onsets. The solution is found from the Euler equation for Lagrangean of the smoothing functional as a Cauchy problem; the initial conditions are determined by the “mask” method. A technique for determination of hazardous zones relying on comparison of the model in the planetary rover and of the actual scene is described that uses a “language” aproach combined with the gradient method. The action of the algorithms in a specific scene is described.
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