A CCD detector attached to the lower latitude meridian circle. (III) Several correction for the spherical astronomy.

Details A CCD detector attached to the lower latitude meridian circle. (III) Several correction for the spherical astronomy. A CCD detector attached to the lower latitude meridian circle. (III) Several correction for the spherical astronomy.

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pyuno...1...77h&link_type=abstract

Publications of the Yunnan Observatory, No. 1, p. 77 - 86

Physics

Scientific paper

The curvature correction, which should be added to the determined value of the zenith distance in the meridian direction, and the corresponding corrections of the time of a star's passage across the prime vertical direction and of the determined value of the zenith distance are derived by means of the method of the projection ellipse. The influence of the variation in the angle between the projection of the right ascension circle of an object and the meridian plane on the determined value of the measured coordinate during the observation of the star carried out in the meridian direction is also derived.

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