... Space Research Institute . Main . ... Main results of the experimental and theoretical research completed in 2010 . ... Moon's topography is shown based on LOLA laser altimeter data, white contour shows a permanently shadowed region and a white rhomb indicates LCROSS spacecraft impact location. ... Ultra deep survey of the sky in hard X-rays, performed by INTEGRAL observatory . INTEGRAL observatory has completed the first and the most sensitive survey of the sky in hard X-ray energy band. ...

Organizing Committee . Scientific Topics . ... Scientific Programm . ... Ulyanovsk . ... International Advisory Committee . Chairman Prof. M.V. Sazhin . e-mail: sazhin@sai.msu.ru . ... Prof. V.N. Lukash . e-mail: lukash@dpc.asc.rssi.ru . Vice-Chairman, Chairman of the Local Organising Committee: . Prof. S.V. Chervon . e-mail: chervon@sv.uven.ru . ... TEL: 007 (095) 939 5006 . ... E-MAIL: alexeyev@grg2.phys.msu.su . ... Theoretical and Mathematical Physics Departament, . ...

... The Russian Federation State Program "Physics of Condenced Matter", the "Superconductivity" division , Project code "Generation-2" . ... The multielement josephson structures are known to allow implementation of the unique properties of the Josephson junctions as electromagnetic waves sources with high change rate of generation frequency, working in the millimeter and submillimeter wavelength diapasones. ... Even the optimal type of the junction electrodynamic interconnection isn't chosen. ...

... This file table3 82 660 Observed wavelengths, laboratory values and identifications -------------------------------------------------------------------------------- Byte-by-byte Description ... Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- SpOrd Spectrum order 5- 12 F8.3 0.1nm SolLam Wavelength determination of all solar and telluric lines measurable on the ... Note (6): J: Junkes et al., ...

Building the Foundation for U.S . Astronomy at m/cm Wavelengths in 2010 and Beyond Community Workshop (*) Workshop SOC/LOC Robert Brown (NAIC) Chris Carilli (NRAO) Jim Cordes (US SKA Consortium) Dale Frail (NRAO) B. Murray Lewis (NAIC) K. Y. Lo (NRAO) Emmanuel Momjian (NAIC) Yervant Terzian (US SKA Consortium) (Special thanks to Billie Rodriguez, Jill Tarbell and Joan Martin) * Support provided by NSF, NRAO, and NAIC R. L ...

... Contemporary State ol SETI Problem In Russia . ... Presently the scientific and technological civilization on Earth possesses only one method of searching for extraterrestrial civilizations in outer space - the method of remote observation by scanning, optical and radio data from the surrounding space and by trying to detect and. recognize possibly intelligent signals. ... Theoretical Foundations ot the Contact oi Intelligent System. ... Intermediary Languages for the Contact ot Intelligent Systems....

. False color image of the galaxy LAEJ095950.99+021219.1. In this image, blue corresponds to optical light (wavelength near 500 nm), red to near-infrared light (wavelength near 920 nm), and green to the narrow range of wavelengths admitted by the narrow bandpass filter (around 968 nm). LAEJ095950.99+021219.1 appears as the green source near the center of the image cutout. The image shows about 1/6000 of the area that was surveyed. Photo credit: James Rhoads

The last few years have seen a transformation in our understanding of the formation and evolution of galaxies. ... In the years ahead, new facilities like the JWST, CCAT, the LMT, ALMA, the JVLA, LOFAR and the SKA will shed further light on how galaxies form by providing huge increases in sensitivity over five decades in wavelength: from the near-infrared to long radio-wavelengths. ... AGN and Galaxy Evolution . Gas in Galaxies . The High-redshift Universe and the First Galaxies . ...

... Under certain conditions, like those in the nucleus of a QSO, all atoms can be made to emit light at particular wavelengths. ... If that source is approaching the observer, the wave is squashed up onto itself making the wavelength shorter. ... This is redshift. ... You can see how the section of the QSO spectrum which we observe changes with redshift. ... We then see how far we had to slide the observed spectrum along the scale to make it match and that is the objects redshift. ... The 2QZ team . ...

... Particle Sizes in Saturns Rings . ... Credit Copyright: RSS , JPL , ESA , NASA Explanation: What size particles compose Saturn's rings? To help find out, the robot Cassini spacecraft now orbiting Saturn broadcast radio waves of three different wavelengths right through the rings to Earth earlier this month. The experiment was sensitive to ring particle sizes because ring particles much larger than a broadcast radio wavelength will reflect those radio waves away. ... NASA Official: Jay Norris. ...

... Schools . ... Dean?s Office . Departments . ... Applied Chemistry Department . ... Theoretical and Applied Systems Engineering Department . ... Economic Cybernetics and Applied Economics Department . ... School of History . ... Ancient and Medieval History Department . ... History ofљEastern Europe Department . Modern and Contemporary History Department . Ukrainian History Department . ... University History Museum . ... History of Russian Literature Department . ... School of Physics . ...

... 1 - 5 m HgCdTe Detector Material . Hybridization of 2048 x 2048 Arrays . ... Options for Extension to Visible Wavelengths . ... MBE HgCdTe Capability at Rockwell Science Center . ... Over the last two decades, dramatic improvements in the performance of 1 - 5 m infrared detector materials combined with the leap from single detectors to million pixel arrays have led to a billion-fold improvement in our ability to observe astronomical sources at these wavelengths. ...

... Before the modern era of technological astronomy, to know anything about the Universe beyond our planet we relied on light. ... Historically the two rival ideas were that light was either a stream of tiny bullet-like particles or a wave wobbling its way through space. ... The light we see (visible light which is not the tautology it sounds) is only part of the electromagnetic spectrum, a great sweep of radiations which also includes radio, infra-red, ultra-violet, x-rays and gamma rays. ...

Perhaps the greatest theoretical achievement of physics in the 19th century was the discovery of electromagnetic waves. ... It is possible to use this to define a unit of electric charge, as the charge which repels a similar charge at a distance of, say, 1 meter, with a force of unit strength (actual formulas make this precise). ... But "field" originally only meant the force a magnet or an electric charge could expect at a point in space, if it were placed there. ...

... They cover a period of 4 days in which the Supernova continues to rise in brightness (what astronomers call magntiude). ... First Image Taken on March 11 at 8:22 UT. Second Image Taken on March 12 at 8:52 UT. ... The supernova is the same brightness as in the previous image taken 2 hours ago . ... This image, taken 24 hours after the previous image, shows the supernova to be another 0.21mag (or about 25%) brighter. ... Hopefully the images do show that the brightness of the Supernova is changing. ...

OJC «RPC «Precision Systems and Instruments», Moscow, Russia A. Alexandrov, V. Shargorodskiy On the possibility to create a prototype of laser system for space debris movement control on the basis of the 3-meter telescope. ... Large number of theoretical works, which are devoted to laser method of impact on SD, consider light pressure and material removal (evaporation, ablation) for thrust generation. ... Laser ablation is the process of removing material from a solid surface due to laser spark). ...

Teoretical Astrophysical Center and Astronomy Group in Aarhus . ... Stanford Solar Physics Research Group. ... The Helioseismology Group, ( broken link ) in Institute of Astronomy , Cambridge University . ... GONG - Global Oscillation Network Group (Tucson) . SOHO . ... Large calendar of Astronomy Events . ... SOHO meetings and events . ... CNRS - Les relations internatianalites du CNRS , about Accords De Cooreration Scientifique . ... Solar Physics (Marchal Space Fligth Center) science site. ...

... Telescopes . ... Fig. ... Theoretical optical resolving power of the MSS, depending on the phases of the moon under typical weather conditions. ... The optical resolving power of the telescope with the MSS allows to observe stars of up to the 12 magnitude. ... Currently, more than 90% of observational time with the MSS spectrograph is used in the spectropolarimeter mode with a diffraction grating 24.7њ. ... wide spectral region with a reciprocal linear dispersion of 9 ?/mm (0.1215 ?/pix) at a time. ...

... U filter . UG1 - 1mm . S8612 - 2mm . WG295 - 2mm . ... BG37 - 3mm . BG39 - 1mm . GG395 - 1mm . ... GG495 - 2mm . BG40 - 3mm . ... OG570 - 3mm . KG3 - 2mm . ... RG9 - 2mm . WG305 - 3mm . Bessell, PASP 102 , 1181, (1990) . ... Bessell, PASP 107 , 672, (1995) . APO Filters Homepage ...

Born: March, 29 1962 (Moscow) . ... Inst., ... Inst. in 2001. Title of thesis: "Matrix models and geometry" . ... Courses in theoretical mechanics, field theory, and string theory in the College of Mathematical Physics of Independent Moscow University in years 1994--2001. ... Quantum field theory: gauge and supersymmtric theories, matrix models and integrable systems, graph theory. ... By L.O.Chekhov and R.C.Penner Russ.Math.Surv. ... 7) Matrix models versus Seiberg-Witten / Whitham theories. ...