uzbek academy
Recently Published Documents


TOTAL DOCUMENTS

11
(FIVE YEARS 0)

H-INDEX

2
(FIVE YEARS 0)

2001 ◽  
Vol 24 (3) ◽  
pp. 233-233
Author(s):  
Salakhutdin N. Nuritdinov

Our Department of Galactic astronomy and Cosmogony of the Astronomical Institude of Uzbek Academy of Sciences has rich photo meterials obtained over more than 100 years by two telescopes (Normal Astrograph with F= 3500 mm, D= 330 mm and Zeiss Double Astrograph with F= 3000 mm, D= 400 mm). The main objects studied are: 1Open and Globular star clusters,2Regions of the Milky Way and the Pulkovo Observatory program.3Comets and Asteroids4Planets and their Satellites.There are also astronomical data received in the framework of a number of International programmes. Now we are working out some research-complex programmes of these objects. We are ready to collaborate on these programmes.


2000 ◽  
Vol 178 ◽  
pp. 163-168 ◽  
Author(s):  
Sh.A. Ehgamberdiev ◽  
S.K. Eshonkulov ◽  
E.A. Litvinenko

AbstractThe Tashkent Astronomical Observatory (Ulugh Beg Astronomical Institute of the Uzbek Academy of Sciences since 1966) was involved to the International Latitude Service (ILS) in September 1899, when the regular latitude measurements were started at Tschardjui (ϕ = +39°08′11″,λ = −63°29′). Because of the Civil War in Central Asia, the latitude observations were ended at Tschardjui in May, 1919. A new latitude station was established at Kitab (Uzbekistan) at latitude ϕ = +39°08′40″ and longitude λ= −66°53′, in November 1930. The Kitab Latitude Station was equipped with two visual zenith telescopes (1929, 1957) and the photographic zenith tube removed from the Pulkovo observatory in 1978. The Kitab station provided the ILS with more than 250000 instantaneous latitude measurements. Since the early 90s Kitab has hosted the ground-based beacons of GPS, PRARE and DORIS satellite tracking systems, providing the IERS data center with precise coordinates at sub daily frequency.


Sign in / Sign up

Export Citation Format

Share Document