Main Sections LabIR main page . ... On January 23, 1998 the space probe NEAR was on its way to its closest approach to Earth. ... However, we were able to record a series of images of the space probe shortly before the sunglint event, and we have assembled them into a movie. At the TIRGO observatory, an observation of the space probe NEAR was organized for the night of January 22-23, 1998. ... We show here a preliminary movie (MPEG format, 412kb) made from 74 frames, each lasting 5 seconds. ...

... License agreement. All copyrights to Izmccd are exclusively owned by the author- Igor Izmailov. ... THE AUTHOR WILL NOT BE LIABLE FOR DATA LOSS, DAMAGES, LOSS OF PROFITS OR ANY OTHER KIND OF LOSS WHILE USING OR MISUSING THIS SOFTWARE. You may not use, copy, emulate, clone, rent, lease, sell, modify, decompile, disassemble, otherwise reverse engineer, or transfer the licensed program, or any subset of the licensed program, except as  provided for in this agreement.  ... Igor Izmailov. ...

... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...

. at the 48 aud. of the Sternberg Astronomical Institute, . at 14 00 on Friday, December 9 , 2005 . (113-th seminar) . 1. L.G.Lukyanov (SAI) . "Modified Roche lobe for eccentic binaries" . 45 min . 2. News . The secretary of the seminar - M.E.Prokhorov . Access free (code 2197) . Abstracts and INTERNET Subscribe possible at . http://xray.sai.msu.ru/sciwork/eseminars.html .

. Astrophysics Group . Cavendish Laboratory . Department of Physics > Astrophysics . Home . Programme . Venue . Registration . Organisation . Accommodation . Participants . Talks . Photos . The workshop will be hosted at the new Kavli Institute for Cosmology , Cambridge, located alongside the Institute of Astronomy . Directions are available here . Last modified: 8 August 2009 . 2009 Astrophysics Group, Department of Physics, Cavendish Laboratory, University of Cambridge . Information provided by webman

Numerical simulation of the self-pump ed Long Josephson junction using a modified Sine-Gordon model A.S. Sobolev a,, A.L. Pankratov b, J. Mygind a c Institute of Radio Engineering and Electronics (IREE), Mokhovaya st. 11/7, Moscow, 125009, Russia b Institute for Physics of Microstructures of RAS, Nizhny Novgorod, Russia c The Danish Technical University, Kgs. ... In our model the dumping parameter dep ends b oth on the spatial coordinate and the amplitude of the AC voltage. ...

The SAOtng graphical user interface is written in TCL using the NOAO widget server . A copy of the GUI specification is maintained in a file named saotng.gui , available in the SAOtng bin directory. If you are familiar with TCL, you can modify this file to create a new GUI and use it as your SAOtng interface. ... But if you create a modified version of saotng.gui, use: make crunch in the SAOtng directory to create the crunch.gui file. ...

... the radiative transfer equation (RTE) for the randomly-irregular magnetized plasma has been derived on the base of general grounds of the multiple scattering theory . ... Solutions of several absolute tasks of the scattering theory have been obtained (on the optical depth of the ionospheric plasma layer, on the value of radio wave anomalous attenuation, on anomalous refraction, on the backscattered signal intensity for the source being placed within a plasma layer). ...