|
Maidanak Observatory (66°56' E, 38°41' N) is located at the south-east
of the Republic of Uzbekistan. It lies on the spurs of the Pamir
Alai mountain system at 2000 m above sea level. This summit was
selected for astronomical observations in the late 60-s a result
of a ten-year long site assessment campaign organized at the Ulugh
Beg Astronomical Institute (UBAI) of the Uzbek Academy of Sciences.
The studies of the Mt. Maidanak astroclimate continued through
the 80-s and up to the beginning of the 90-s by several groups of
researchers using different methods and instruments. But those groups
give different values of seeing due to the limitation of the methods
and systematic errors of the instruments used. Seeing measurements
with a Differential Image Motion Monitor (DIMM), designed by the
European Southern Observatory (ESO) and used to estimate the seeing
at the La Silla and Paranal Observatories in Chile have been carrying
out at Mt. Maidanak since August 1996. The median value of the seeing
at Mt. Maidanak for the last three years of observations is 0.69
arcsec. For the La Silla and Paranal Observatories, the value of
this parameter are 0.87 and 0.66 arcsec, respectively. It is indicated
that Mt. Maidanak is one of the most favourable site for astronomical
observations.
When the high-quality atmospheric conditions of Mt. Maidanak were
established with a modern instrumentation, the next step was to
measure other atmospheric parameters relevant to adaptive optics
and interferometry, such as wavefront outer scale, isoplanatic angle,
high altitude wind. In July 1998 during a site testing campaign,
supported by INTAS-096-37 grant, all these parameters were measured
with the Generalized Seeing Monitor (GSM) developed at the University
of Nice.
Comparison of the all these atmospheric parameters of Mt. Maidanak
with ones at other well known observatories show that Mt. Maidanak
is a favorable site for future installation of an extremely large
telescopes. Exeptional futures of Mt. Maidanak are very low wind
speed and geographical location at middistance between two international
astronomical facilities at Canaries and Hawaii.
Home page
|