Discussion of the results from solar astrolabes

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astrometry, Reference System, Sun: General, Methods: Data Analysis

Scientific paper

In this work we investigate on the stability of the results from solar observations obtained with the modified astrolabes of the Observatoire de la Cote d'Azur/France, of the Observatorio Abrahao de Moraes/IAG/USP-Brazil and of the Observatorio Nacional/Brazil. The mass of data is comprised of 6273 observations of both solar limbs, from 1974 to 1992, and is analyzed to determine the origin of the fundamental reference system and the Earth's orbital parameters. The solution stability was verified by checking against any large variation upon the individual weights, as well as for differentsamples of the whole set of observations. The results were also shown invariant to changes in the adopted model, such as adding unknowns to the refraction algorithm, to the time variation of the obliquity (including the nutation constant) and to the azimuthal anomalies of the refraction. In our analysis we obtain a standard deviation of 0.6" for the combination of the observations with no bias on its distribution. It is also indicated that the Sun observations at astrolabes do not require any further atmosphere modelling complexity.

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