New method for reduction of astrolabe observations using rectangular coordinates on the celestial sphere

Details New method for reduction of astrolabe observations using rectangular coordinates on the celestial sphere New method for reduction of astrolabe observations using rectangular coordinates on the celestial sphere

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985bgeod..59..391k&link_type=abstract

Bulletin Géodésique, Volume 59, Issue 4, pp.391-395

Statistics

Scientific paper

A new reduction method using x, y, z-coordinates is derived for astrolabe observations. By this method, the latitude and the longitude of the station are computed without the need of a priori knowledge of the station position. This method is a significant development in data reduction of astrolabe and other almucantar observations due to its mathematical exactness, simplicity, and the ease of handling the associated statistics.

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