Abstract
The approach described in this paper allows the numerical calculation of the gravity of two- and three-dimensional bodies, provided their boundaries can be expressed by two single valued functions. Boundary integral theorems are used to convert the integrals for the gravity components into a form which can be integrated numerically. To perform numerical integration routines based on the Gauβ quadrature method are applied.
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More From: Archives for Meteorology, Geophysics, and Bioclimatology Series A
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