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.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callMore From: Archives for Meteorology, Geophysics, and Bioclimatology Series A
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
