Abstract

Various forms of geophysical modeling require a technique for computing the gravitational attraction of a specified source distribution of mass. I show in this paper that the triple integral that arises in general gravitational modeling can, under certain conditions, be reduced to a single line integral or even to a finite sum.

This content is PDF only. Please click on the PDF icon to access.

First Page Preview

First page PDF preview
You do not currently have access to this article.