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), ...

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 . ...

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. ...

... 314 ­ 321 Non­LTE Line Formation for Fe I and Fe I I in the Atmospheres of A­F Typ e Stars Mashonkina L. Institute of Astronomy, Moscow, Russia Abstract. ... Non­LTE leads to the Fe II lines strengthening, however, the effect is small, such that the abundance correction is at the level of -0.01 to -0.03 dex over the whole range of stellar parameters being considered. ... 2 What is Meant by the Non­LTE Approach? ... For the Fe I lines, we obtained the mean non­LTE abundance log FeI = 7.56 ± 0.09. ...

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