... Russian Foundation for Basic Research , Project number 98-02-17366 . ... A number of experiments proposes the d -type of the wave function, having two directions with positive and two (in orthogonal direction) - with negative sign of the order parameter. ... The effect of the wave function phase is most efficiently revealed in the experiments with Josephson structures, that are used for determination of the dependences on the pulse direction. ... The project goals are: . ...

Current Opinion in Solid State and Materials Science 5 ( 2001 ) 9 ­ 14 Grain boundary migration: misorientation dependence G. Gottstein a, *, D.A. Molodov a , L.S. Shvindlerman a , b , D.J. Srolovitz c , M. Winning b c a a Ё Institut f ur Metallkunde und Metallphysik, RWTH Aachen, Kopernikusstr. ... An example is shown in Fig. 1, where the misorientation dependence of GB mobility ] b 5 A 0 exp(2Hm / A kT ) and its parameters for tilt GBs in pure aluminium ( 99.9995 at% ) is presented [**1]. ... Fig. ...

... Gallery . Simulation Images . Simulations of convection in stars . Side-view of the temperatures in a simulationтАж . Sidebar Left . Sidebar Top . No Sidebar . Sidebar Bottom . Sidebar Right . ... Title: Side-view of the temperatures in a simulation of a white dwarf . ... NOTE: All images are copyright and must not be reproduced or mirrored in any form without written permission. ... Side-view of the temperatures in a simulation of a white dwarf €йRegner Trampedach . ...

The study of energetic particles acceleration and transport within the magnetosphere and on its boundaries is the main goal of DOK-2 experiment on Auroral Probe in a frame of INTERBALL project. ... DOK-2 uses two pairs of energetic particle telescopes . ... This information is available only during the most informative Real Time mode of DOK-2. ... Full 56-57 channel spectra accumulated during time intervals from 10 s to 1464 s depending on a particle intensity. ... For this time interval: . ...

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... Flights Chronology . ... Project History . ISS Russian Segment . Steps of ISS Assembly . ... Monitoring both the state of experimental cells with media investigated and provision of thermal contacts by all temperature sensors having an effect on SE results interpretation. ... HISTORY . ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

ENERGETIC PARTICLE EXPERIMENT DOK-2 . ... Due to much higher energy, angular and time resolution, better separation of electrons and ions it is expected that DOK-2 experiment will allow to re-examine in more details energetic particle population and related processes in magnetosphere regions covered by the spacecraft orbit. ... Thin foil in front of detector absorbes protons with energies E<400 keV so this detector measures electron spectrum in 20 - 420 keV range. ... Energy values, keV . ...

Subject, Object and Problems of Astrophysics. Practical and Theoretical Astrophysics. ... Visual Telescope; Problems Which Are Solved with the Its Help. ... Resolution of Telescopes. ... Effectiveness of Telescope in Respect of Resolution. ... Optical Power of Telescopes for Star-like and Extensive Objects. Boundary Magnitude. Reasons of Light Dissipation in Telescopes. ... Spectral Instruments in Astrophysics. ... Basic Photometrical Ideas, Magnitudes and Their Measurement. ...

... The problems of complexity in coagulation: specification 1. ... Numerical experiments Task 1: Activation threshold Final clot density VS activation : model reduction Factor V is activated 7 6 7 6 No factor V activation Fibrin 4 3 2 1 0 0.00 0.02 0.04 0.06 0.08 0.10 0.12 Fibrin 5 5 4 3 2 1 0 0.00 0.02 0.04 0.06 0.08 0.10 0.12 Activation Activation y= Ae ( Bx 1 ) y = Ax Final clot density VS activation : the experiment Fibrin clot density (a.u.) 1.0 0.8 0.6 0.4 0.2 ...

... EXPERIMENT COLD: . THE FIRST DEEP SKY SURVEY WITH . THE RATAN-600 RADIO TELESCOPE . ... 2 The RATAN-600 Radio Telescope . ... 2.2 Brief Description of the RATAN-600 Radio Telescope . ... Elimination of Discrete Sources . ... Sky Surveys Using the RATAN-600 . ... 5 Astrophysical Problems Studied in Experiment Cold . ... Point Sources, i.e., on Scales Comparable to the Beam of the Radio Telescope . ... Strong" Radio Sources . ... Experiment Cold and the "New-Generation" Radio A stronomy . ...

Physics Colloquium Dec 21, 2000 . LCWS 2000 Oct 22-28, 2000 . Univ. of Idaho Colloquium Oct 13, 2000 . ICHEP July 27-August 2, 2000 . APS Meeting April 29 - May 2, 2000 . Berkeley 2000 March 29-31, 2000 . LSC March 16-18, 2000 . ... Talks 2003 . ... Talks 2002 . ... Talks 2001 . ... Talks 1999 . ... Study of energy Flow in Jet Reconstruction , Ray Frey, Masako Iwasaki . ... Experimental Study of Neutron Radiation damage in CCD Detectors , Nikolai Sinev, Jim Brau . ...

... We present methods of comparing theoretical predictions for the anisotropy of the Cosmic Microwave Background Radiation (CMBR), with the results of various experiments. ... Temperature flucuations . ... Most models of structure formation in the universe predict anisotropies in the CMBR. ... Therefore one must take into account not only the theoretically expected value of the temperature fluctuation but also the so-called cosmic variance, i.e. the theoretical error due to observing only one universe....

26aug00 ,2000 A temperature sensor is mounted above the IF/LO racks on the rotary floor (in the dome). ... The temperature in the rotary floor room had risen from 74 degF to 82 degF. The air conditioning in the room got the temperature back down to 74 degF at 6:00 hours. ... There is also gain downstairs. ... The current air conditioning needs about 3 hours to get the rotary floor room back to the normal temperature after a nighttime sband xmit experiment (when the air temperature is 73 degF). ...

... This thread uses PINTofALE to generate a simulated Chandra spectrum. ... define a DEM . ... pset marx .par ExposureTime=50000 OutputDir='sim_ marx ' \ ; GratingType='NONE' DetectorType=' ACIS-I ' SourceFlux=-1 \ ; SpectrumType='FILE' SpectrumFile='spec_ marx .dat' \ ; SourceType='POINT' DitherModel='INTERNAL' ; marx TSTART=2006.46 ; marx2fits sim_ marx / spec_ marx .evt ; dmextract infile= spec_ marx .evt[EVENTS][(x,y)=circle(4018,4141,10)] ; [bin pi=1:1024:1] outfile= spec_ ...

... Light sources: POV-Ray works with point sources of light. ... A real star consists of a spherical light source (the photosphere where the continuum is formed) superimposed by a scattering layer (an atmosphere) responsible for phenomena such as limb darkening and absorption lines. ... For example, in order for the central light source to illuminate the surface, the star must be transparent. ... The POVRay source for creating the white dwarf binary merger movie is given for demonstration purposes. ...

Star Colors in Orion . ... Credit Copyright: Jens Hackmann Explanation: What determines a star's color ? ... Red stars are cool, with surface temperatures of around 3,000 kelvins (K) , while blue stars are hotter and can have temperatures over 30,000 K. Our own lovely "yellow" Sun's temperature is a comforting 6,000 K. Differences in star colors are particularly easy to see in this intriguing composite view of the constellation Orion, made while experimenting with a star trail step-focus technique . ...

... We computed the permanently shadowed areas and temperatures inside the craters for the variation of the position of the lunar pole of rotation with respect to the ecliptic pole with a period of 18.6 years. ... According to our results, the total permanently shadowed area in the polar craters of the Moon is equal to 50428.7 km2, or 0.13% of the total area of the lunar surface [3]. ... The area of permanently shaded part of a crater makes 59 % from all area of a crater [3]. ...

... You are here: start €Ё lbaops €Ё lbamar2013 €Ё v255r . ... VLBI Schedule . ... Observer's Wiki . ... lbaops:lbamar2013:v255r . ... Channel 1 . IFP#1-LO 6300 - 6316 MHz USB RCP . ... IFP#2-LO 6642 - 6658 MHz USB LCP . ... IFP#2-HI 6658 - 6674 MHz USB LCP . ... 6316 & 6658 MHz . ... 6642 - 6658 MHz USB RCP . ... 6642 - 6658 MHz USB LCP . ... 6658 - 6674 MHz USB RCP . ... 6658 - 6674 MHz USB LCP . ... IFP#1-LO 6642 - 6658 MHz USB RCP . ... Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v255/v255r . ...

. ASME Paper 95-GT-437. Jacques Lewalle, jlewalle@syr.edu

... 2006 March 13 . Z Machine Sets Unexpected Earth Temperature Record . ... The plasma reached a temperature in excess of two billion Kelvin , making it arguably the hottest human made thing ever in the history of the Earth and, for a brief time, hotter than the interiors of stars. ... During the unexpected powerful contained explosion, the Z machine released about 80 times the world's entire electrical power usage for a brief fraction of a second. ... About APOD | ...

... ALFA LIDAR experiment . ... Center for Astronomical Adaptive Optics: measurements of the Atomic Sodium Column Density . ... First Sodium Laser Beacon at La Palma ING Newsletter , March 2000 . ... Ageorges N., Hubin N., 2000, A 144, 533-540 Atmospheric sodium monitor for Laser Guide Star Adaptive Optics , see also other related publications . ... Laser guide star adaptive optics: measuring the sodium column density using a magneto-optical filter , PATRIARCHI P., CACCIANI A ( PDF ) . ...