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Method of A. A. Rambaut The methods of A.A. Rambaut is based on the measurement of one star and and the reduction of the movement in both directions, the declination and th rightascension. Where in the sky The declination and the local hour angle can be chosen at will with the exception of the celestial equator and the neighboring region. On the celestial equator the method fails completely. Is the star trail in one of the directions small then choose a star which has a hour angle which differs about 90o. Alignment of the measurement filed and orientation of the axes The alignment of the measurement field is equatorial. The positive x-axis points in the direction of the positive rightascension, that means toward East. The positive y-axis points in the direction of the negative declination, that means towards the South. Duration of the measurement The duration varies between 10 and 120 minutes. Zero point The zero point is the true celestial pole. After the alignment the hour axis has to be lifted by the value Rb towards the zenith. Procedure
After the star has been centered it is time to track the star without any intervention. Read the position after about 30 minutes on the measurement field. Enter both values X and Y in the fields X direction and Y direction in units of the grid. Enter the measurement duration in seconds into the field Observing period. Enter into the field Resolution per unit the grid unit in arc seconds and hit submit. Example With the following parameters Latitude:
+47 you obtain the following results Rambaut
A : -114.07 arcsec
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Comments, questions, corrections? markus.wildi@one-arcsec.org |
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