
Abstract
Surveying instrument such as theodolites and tracking interferometers are designed to be operated in an upright position. There is typically an alidade with a single azimuth bearing and a laser or telescope trunnion having two bearing for the elevation axis. When operated in an upright position the center of gravity (CG) is over the azimuth bearing and is essentially a compressive load. In a non-upright position the CG shifts off the bearing. Once the CG is not over the azimuth bearing the loads change to tension and shear loads. Depending on the bearing preload during its construction the bearing can "open up" and cause imperfection in the "vertical" axis through the instrument, in what herein is called "gravitational droop". This paper analyses gravitational droop which is a function of gravitational direction and azimuth angle, creating bias error in the measured space.
Also published as CMSJ-12-2-04, The Journal of the CMSC, Volume 12, Number 2 (Autumn 2017).
Cite this paper
John W. Dorsey-Palmateer. JDP Metrology Consulting, LLC, Gig Harbor, WA. Presented at the Coordinate Metrology Systems Conference 2017, Snowbird, Utah, July 17-21, 2017. Coordinate Metrology Society, reference CMS-2017-015.
