A Numerical Approach for Solving the System of Differential Equations Related to the Spherical Curves in Euclidean 3-Space

Abstract

In 1971, integral form of spherical curve in 3-dimensional Euclidean space was given in [3]. Theexplicit characterization of the spherical curves in n-dimensional Euclidean space was given in [12]. Morever, theposition vector of spherical curves in Euclidean 3-space was determined in [10]. In the present work, a) it is giventhe system of differential equations of the spherical curves in 3-dimensional Euclidean space; b) it is shown that thenumerical solutions of this system of differential equations are obtained in the truncated Taylor series form by usingTaylor matris collocation method; c) an example together with error analysis are given to demonstrate the validityand applicability of present method.