Astro-Azimuth Using Time Difference

Conventionally, the determination of astronomic azimuth involves the synchronization of the observations with a radio time signal or the measurement of zenith distances which are subject to refraction errors. A mathematical model is developed which is dependent upon time differences (not absolute ti...

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Veröffentlicht in:Journal of surveying engineering 1984-08, Vol.110 (2), p.112-118
Hauptverfasser: Vonderohe, Alan P, Mezera, David F
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container_title Journal of surveying engineering
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description Conventionally, the determination of astronomic azimuth involves the synchronization of the observations with a radio time signal or the measurement of zenith distances which are subject to refraction errors. A mathematical model is developed which is dependent upon time differences (not absolute time) and horizontal angles (nearly refraction-free) between pairs of stars. Error analysis indicates that an optimum star pair includes Polaris and any second star whose azimuth is at least moderately changing. Field tests indicate that the azimuth of Polaris may be determined to within 0.6 seconds of arc. The formation and solution of the necessary equation may be implemented on a programmable calculator.
doi_str_mv 10.1061/(ASCE)0733-9453(1984)110:2(112)
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ispartof Journal of surveying engineering, 1984-08, Vol.110 (2), p.112-118
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1943-5428
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source American Society of Civil Engineers:NESLI2:Journals:2014
subjects Earth, ocean, space
Exact sciences and technology
External geophysics
Geodesy and gravity
TECHNICAL PAPERS
title Astro-Azimuth Using Time Difference
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