... National Astronomical Observatories of China) Kislovodsk 8.10.2010 Wang Hongshuai Kislovodsk Oct.2010 2 2008.11 Oma Site 40 m CT 2 tow er 4.5 m antenna Satellite communication w eather station 10m tow er SBIG seeing m onitor DIMM seeing dome MIR cloud ...
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Ссылки http://site2010.sai.msu.ru/static/doc/WHongshuai_site2010.pdf -- 1237.0 Кб -- 20.10.2010 Похожие документы
... of the upper one was mainly 3.10 m (points 912 in Fig. 1, 2.55 m for point 8 ... points µ m. Asymptotic similarity relations = { , m (µ ) = = , = 2.503, = 4.669. 8 ...
... 2% for a 2 minute exposure on a 30" FoV at = 1 m Differential Astrometry 50 mas for ... Mauna Kea conditions Altitude (km) Wind Speed (m/s) 0 5.6 0.5 5.8 1 6.22 7.6 4 13 8 ...
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Ссылки http://site2010.sai.msu.ru/static/doc/GHerriot_site2010.ppt.pdf -- 1942.1 Кб -- 18.10.2010 Похожие документы
... With this device have been made optical tests for 6 telescopes from 0.7 to 2.6 m. In all cases it is possible to receive an estimation dome seeng for slow (quasistationary) streams . ...
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Ссылки http://site2010.sai.msu.ru/static/doc/SPotanin_site2010.pdf -- 522.6 Кб -- 31.10.2010 Похожие документы
... According to (2), (V)med(M(z)=1) = 0.945". and R AZT-22 data ((V) and Since, strictly speaking, (2) is valid only for the free (R), reduced to unit air mass) atmosphere, our estimate of (V)med(M(z)=1) should be for the same nights, averaged treated ...
... down to nanoJansky level) in a single dish mode, and observations with high angular resolution in the interferometer mode. · main reflector diameter 12 m, cooled to 4.2 K · HEB mixers for 1 6 THz http://www.asc.rssi.ru/millimetron/eng/millim_eng.htm ...