Differential measurement method for atmospheric refraction and the results of experimental observations

Astronomy and Astrophysics – Astronomy

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Atmospheric Effects, Astrometry

Scientific paper

Because of the effect of the atmospheric refraction, it is seldom to observe objects with altitude lower than 15 degree. But for the complete theoretical research of the atmospheric refraction, it is necessary to observe such objects, even with altitude close to 0 degree. Especially in some special situation, some objects with low altitude need to be observed. A new differential method is presented to measure the atmospheric refraction. Starting with the zenith, a series of star fields at different altitude are observed by a telescope with larger field of view, the derivatives of various orders are calculated at different zenith distances, and finally the observational atmospheric refraction can be obtained by numerical integration. The method does not depend on strict local parameters and precise instruments, while the observational principle is relatively simple. An experimental observation was carried out with a simple telescope with large field of view at Xinglong station of NAOC at the end of 2007. The atmospheric refraction from the zenith distance of 44.8 degree to 87.5 degree is gotten by the differential method, which proves the feasibility of the method tentatively. Limited by the observation condition, the precision of the result is not high. The maximal accidental error is about 6 arc second, and there is also some systematic error. The difference between the observation atmospheric refraction and Pulkovo table is about 15 arc second at the zenith distance of 84 degree. How to eliminate the accumulated errors introduced by the errors of the integration model is the key problem that needs solving in the future.

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