Global method for astronomical determination of geographic coordinates in the C.I.O. system
A method for direct determination in the Conventional International Origin System (C.I.O.) of GEOGRAPHIC LONGITUDE AND LATITUDE from a topocentric place is discussed. Simultaneous measurements of time (U.T.C.) and zenith distance of three non-specified celestial bodies (with well-known equatorial ap...
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1988
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| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/142185 |
| Aporte de: |
| Sumario: | A method for direct determination in the Conventional International Origin System (C.I.O.) of GEOGRAPHIC LONGITUDE AND LATITUDE from a topocentric place is discussed. Simultaneous measurements of time (U.T.C.) and zenith distance of three non-specified celestial bodies (with well-known equatorial apparent coordinates) must be taken, within a short lapse. It does not demand a special observation program and the Gauss, Zinger and Pewsow methods may be derived as particular cases from the method here considered. |
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