18.10.01 / jn
For some new observational methods it is necessary to
use the telescope
coordinate system (azimuth/elevation), but also have these positions
corrected
for the pointing errors. Specially that is useful for example to
observe
around the pole or to exactly point geostationary satellites without
having
their movements in the sky.
For that reason we changed the coordinate system
10:
SBAS 10 is
the same as before ( actual telescope positions in azimuth and
elevation)
SBAS 10 D now works as
descriptive system, but with the pointing corrections
applied
