Mobile Device to Digitize the photographic plates: first results Grosheva E.A., Izmailov I.S., Khrutskaya E.V. Pulkovo Astronomical Observatory, Russian Academy of Sciences, St. Petersburg, Russia Abstract -- The first results of astrometrical reduction for 40 Saturn and Pluto's plates are presented. ... This method of digitization and astrometric reduction of photographic plates using a digital camera is developed due to the problem of plate archive transportation to the high-tech measuring machines. ...

... 2010-01-20 . ... 2011 -01-28 . ... 2012-01-11 . ... 2013-01-05 . ...

... Data Usage Policy . ... Export main Table and RATAN-600 data . ... RATAN data . ... Blazar type . ... Data explorer . ... LSP . BLac . RBL . ... BL~Lac . ... BL~Lac~cand. ... ISP . ... XBL . ... BLac.can . ...

TOPEX/Poseidon Jason-1 , , 14-17 2005 . ... 14-17 2005 . ... 110° 90°W. , , 14-17 2005 . ... 25° 25° 30° 30° 35° 35° 40° 40° 1.1993 1.1994 1.1995 1.1996 1.1997 1.1998 1.1999 1.2000 1.2001 1.2002 45° 1.2003 45° -0 .05 -0 .03 -0 .01 0 .01 0 .03 0 .05 0 .07 0 .09 / - 110°W. , , 14-17 2005 . 25° 25° 30° 30° 35° 35° 40° 40° 1.1993 1.1994 1.1995 1.1996 1.1997 1.1998 1.1999 1.2000 1.2001 1.2002 45° 1.2003 45° -0 .05 -0 .03 -0 .01 0 .01 0 .03 0 .05 0 .07 0 .09 / - 100°W. , , 14-17 2005 . ...

... 53, Moscow, 119991 Russia 2 MoscowPhysicotechnical Institute, Dolgoprudnyi, Moscow oblast, 141700 Russia Received June 15, 2004 ° Abstract--We present a catalog of 100 lines in the wavelength range 280­330 A detected by the RES-C spectroheliograph in solar active regions and flares during the SPIRIT experiment aboard the CORONAS-F orbital station. ... The line intensities recorded during the X3.4 (GOES) solar flare of December 28, 2001, are given. ... The Ca XVIII 302.19 A line is observed. ...

... DHOFAR 304, 305, 306 307: . Dhofar 304, 305, 306 307. ... Dhofar 302, 303, 305, 306 307. ... Dh-304 Dh-025 301, Dh-305, 306 307 Dh-081, 280, 302 303. ... Dh-305, 306 307 Dh-302 303, Dh-302 305 . ... MgO), FeNi (7.8 .% ... 1) (HMS) (FAN). ... FAN, HMS . ... Dh-306 FAN HMS (. ... Dh-305, 306 307 Dh-081, 280, 302 303. ... Dh-302, 303, 305 307 . ... Dh-305 307 Dh-303. Dh-305 307 (. ... Dh-305 (HMS) , Dh-307. ... 1) Dh-025, 301 304 ; 2) Dh-081 280 , , ; 3) Dh-302, 303, 305, 306 307 , Dh-302 305 . ...

from __future__ import division from visual import * scene = display(range=(3.0,3.0,3.0),width=1300,height=800,forward=( 0.2 ,-0.3,-1.0)) water = box( pos =(0,- 0.1 , 0.0 ), length=10, width=3, height= 0.1 , color =( 0.1 , 0.2 ,1.0)) alength = 2.0 theta = 0.1 pos1 = vector (0,0,0.6) barge1 = box( pos = pos1, length = 2, width = 0.5, height = 0.1 , color =(0.6,0.4, 0.2 )) x1 = arrow( pos = pos1+ vector (0, 0.1 ,0), ...

In the Table below the masses of some asteroids which were determined during the last years are listed. ... The listed values were determined from observations of many test bodies by the weighted least square fit for one perturbing mass and corrections to the orbit elements of all used test bodies. ... based on the observations of 98 asteroids (including 50278) with the values of standard error of mass determination less than 3.0 10 -11 M Sun . ... Mass . ... 3) Mass 121 : 0.74 x 10 -11 M Sun ; . ...

. Bright Supernovae - 2007 . This data comes from IAU Circulars and occasionally more data will be provided on IAU 's Astronomical Headlines page. An archive of the 2007 updates to this page is available. This is a list of the supernovae discovered in 2007. For supernovae which are still visible, please look at the main page for the latest data. Note that Extra galactic Novae have been moved to a special Extra galactic novae page . For more information, you can look at the following Supernova Catalogs: .

Available online at www.sciencedirect.com Journal of the European Ceramic Society 29 (2009) 337­345 Single crystalline mullite fibres obtained by the internal crystallisation method: Microstructure and creep resistance S.T. Mileiko , A.V. Serebryakov, V.M. Kiiko, A.A. Kolchin, V.N. Kurlov, N.I. Novokhatskaya Solid State Physics Institute ... A special cross-sectional shapes of the fibres are shown in a series of the micrographs presented below to illustrate fibre microstructures (see Figs. ...

... Не менее интересны были соединения 17 июня 2 года до нашей эры и 13 сентября 1170 года, планета Венера проходит по диску Юпитера. ... В 30-градусном секторе встретятся сразу пять больших планет (Юпитер, Венера и Нептун, Марс, Сатурн) и Луна. ... МЕРКУРИЙ 0.16њ сев. планеты МАРС . ... ВЕНЕРА 0.55њ сев. планеты ЮПИТЕР . ... МЕРКУРИЙ 0.35њ южн. планеты ВЕНЕРА . ... МЕРКУРИЙ 0.13њ сев. планеты ЮПИТЕР Тройное соединение!! ... ВЕНЕРА 0.30њ сев. планеты МАРС . ... МАРС 0.36њ сев. планеты ЮПИТЕР . ...

Общая Астрономическая Конференция > Форумы общей направленности > Общий форум любителей астрономии > Точность любительских позиционных ПЗС наблюдений . ... Просмотр полной версии : Точность любительских позиционных ПЗС наблюдений . ... Публикую здесь письма с обработкой моих ПЗС наблюдений астероидов, в первую очередь потенциально опасных для Земли. ... 7495 114 2000 11 18.857320 4 44 36.739 0.08 +23 29 21.67 -0.09 18.9 27 . 7495 114 2000 11 18.875220 4 44 35.829 0.22 +23 29 17.51 0.16 18.2 24 . ...

... Сидерический . период . ... 0.01 . ... Ссылки . все данные взяты из работы 1, знак . отмечает данные из ссылки 2.) ... Astrometric and Geodetic Properties of Earth and the Solar System'' in Global Earth Physics, A Handbook of Physical Constants, AGU Reference Shelf 1 , American Geophysical Union, Tables 6,7,10. ...

... Soc. 427, 790­805 (2012) doi:10.1111/j.1365-2966.2012.21990.x Ages and abundances in large-scale stellar discs of nearby S0 galaxies O. K. Sil'chenko,1,2 I. S. Proshina,1 A. P. Shulga1 and S. E. Koposov 1 2 3 1,3 Sternberg Astronomical Institute of the Lomonosov Moscow State University, Moscow, Russia Isaac Newton Institute of Chile, Moscow Branch, Moscow, Russia Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 OHA Accepted 2012 August 23. ... S0s fading from spirals. ...

... Number 5721 . ... 8 August 2006 . ... Data file: 5721-t3 . ... IBVS No. ... 2000.0 Max Min Type References h m s o ' m m 780217 V1675 Ori 05 34 23.8 -05 08 16 13.70 ( 0.08 ) Ic INB 072 USNO 780218 V1676 Ori 05 34 23.9 -05 15 40 11.19 ( 0.16 Ic) J INB 072 USNO 780219 V1677 Ori 05 34 24.3 -06 06 56 12.96 ( 0.10 ) Ic INB 072 USNO 780220 V1678 Ori 05 34 25.3 -04 54 39 13.24 ( 0.09 ) Ic INB 072 USNO 780221 V1679 Ori 05 34 26.1 -06 15 33 15.64 ( 0.14 ) Ic INB ... Sgr . ... Ori...

... Date UTC R.A Dec. Distance V.Mag Phase Elong. muRAcosDE muDE Dist_dot h m s h m s o ' au. o o /s /s km/s 8 25 2012 5 32 1.00 22 15 7.44024 -11 30 24.9922 28.984184693 7.83 0.03 179.05 -0.1064E-02 -0.4142E-03 0.69822 8 26 2012 5 32 1.00 22 15 1.18460 -11 31 0.7539 28.984735705 7.83 0.06 178.18 -0.1064E-02 -0.4136E-03 1.20977 8 27 2012 5 32 1.00 22 14 54.93292 -11 31 36.4593 28.985581959 7.83 0.09 177.23 -0.1063E-02 -0.4129E-03 1.72060 8 28 ...

Главная > Все корабли > Буран > Библиография . ... К 23-летию полета "Бурана" . ... Разговор в ЦПКиО им. М.Горького, сентябрь 2011 г. Программа создания многоразовой космической системы (МКС) 11Ф36 "Буран" была самой масштабной в истории отечественной космонавтики. ... В середине 1970-х годов, на заре программы "Буран", предполагалось, что летать наши многоразовые корабли будут много и часто. ... После принятия этого решения программа полетов "Бурана" переходила к кораблю 2.01. ...

... Ответ. ... Для достижения желаемого директору достаточно и трех месяцев: в первый месяц: 10*D, 2*Z1, 2*Z2, 0.001*Z3; во второй месяц: 10*D, 2*Z1, 0.01*Z2, 0.01*Z3; в третий месяц: 10*D, 0.1*Z1, 0.1*Z2, 0.1*Z3; а во все остальные месяцы директор может предлагать проголосовать за предложение: 100*D, 0.01*Z1, 0.01*Z2, 0.01*Z3, что естественно, будет отклоняться замами. ... В царстве 20 городов, которые как-то соединены дорогами, причем из любого города можно проехать в любой другой. ... Других дорог...

... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...

... We show that broadband energy spectra of GRS 1915+105 during all these spectral states can be adequately presented by two bulk motion Comptonization (BMC) components: a hard component (BMC1, photon index 1 = 1.7­3.0) with turnover at high energies and soft thermal component (BMC2, 2 = 2.7­4.2) with characteristic color temperature 1 keV, and the redskewed iron-line (LAOR) component. We also present observable correlations between the index and the normalization of the disk "seed" component. ...