Determining the astronomical refraction and building the radio wave refractive delay model measured (V) - Acquisition of measured apparent zenith distances

Details Determining the astronomical refraction and building the radio wave refractive delay model measured (V) - Acquisition of measured apparent zenith distances Determining the astronomical refraction and building the radio wave refractive delay model measured (V) - Acquisition of measured apparent zenith distances

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005pnaoc...2..265y&link_type=abstract

Astronomical Research and Technology. Publications of National Astronomical Observatories of China (ISSN 1672-7673), Vol. 2, No.

Astronomy and Astrophysics

Astronomy

Astronomical Refraction, Instrumental Error, Apparent Zenith Distance, Determination Accuracy

Scientific paper

The demands on accuracy of measured apparent zenith distances and the necessity of elimination of systematic errors during the time of determining the astronomical refraction and building the radio wave refractive delay corrective model are described concisely. According to the new instrumental error theory, compared with error determination techniques used in foreign high accuracy measurement instruments, measurement techniques of all kinds of major errors used in the special measurement instrument and their achievable accuracies are described. Distribution of stars in video CCD images when observed in different azimuths is also presented.

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