A program of solar astrometry with a modified Danjon astrolabe has been in
progress since 1990 at the National Astronomical Observatory at Cerro Calan
, Santiago, Chile. More than 3200 homogeneous observations have been made v
isually by a single observer at 30 degrees and 60 degrees zenith distances.
Here we present and discuss the results in right ascension, parameter Y an
d apparent solar radius obtained during the period 1998-2000. These results
and those obtained in former years are available in electronic form(star s
tar). After almost 11 years of continuous observations, the most interestin
g aspect of the solar results of the Santiago astrolabe is a significant an
d positive correlation between variations in time of the apparent semidiame
ter of the Sun and solar activity.