Chair of solid state physics . ... The Physics of Phonons . ... In the first part of the course “The Physics of Phonons” the dynamics of atoms in one- and three- dimensional crystalline lattices is considered in detail. The quasiparticle conception in solids, taking phonons as an example, is discussed; creation and annihilation operators of phonons, main properties of acoustic and optical phonons dispersion laws, density of phonon states. ... Crystalline state. ... Acoustic and optical phonons. ...

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• Laboratory of materials for electrochemical technologies ISSP RAS

... Space Res., 12, 265, 1992 planetary magnetic dipole: Mizutani, H., et al., ... Astrobiology, 7, 167, 2007 CME induced H+ ion pick-up loss at 0.05 AU for ` Hot Jupiters ' HD209458 b Mass loss ~1011 g/s even for weak CMEs Mmax strong magn. protection in reality Exoplanet magnetospheres - importance of magnetodisk Relatively large amount of observed Hot Jupiters (27%): survival of close-in giants indicates their efficient protection against of extreme plasma and radiation conditions ...

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• http://solarwind.cosmos.ru/txt/2011/presentations/Sun/Ishkov/apj_691_2_1222.pdf

... Field size . Object name . ... Map size . ... Field size: the approximate size of the map in the Y direction. ... Galaxies: . ... Galaxies, which size exceeds some value depending on the field and map sizes, are displayed with their real positional angles and sizes by 25m isophote. ... In the "tools" fields there are links to the several famous AVO (Astrophysical Virtual Observatory) resources: NED and Simbad databases and DSS2 (Palomar Digitized Sky Survey) images of the corresponding sky area. ...

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• Journal "Peremennye Zvezdy"
• Астронет > Archive of Astronomical and Astrophysical Transactions
• Evolution of the Moon

... A.V. Eliseev . ... V.V. Adushkin, A.V. Vityazev, D.O. Glazachev, G.V. Pechernikova . Exogenous factors in the evolution of the Earth. ... Cosmic rays as a factor of biospheric evolution . ... A.V. Yakushev, N.A. Churilin, V.S. Soina, A.G. Kudinova, E.A. Vorobyova, N.S. Mergelov . ...

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• Passing arguments to the shell
• Creating a distribution list
• Models recipes

... at the IITP. 1993-1995: researcher at Moscow International Mathematical Institut. a) Mathematics: Theory of Probability, Random Processes , Mathematical Physics, Theory of Interacted Particle Systems. b) Queueing Theory: Queueing Networks , application of the Theory of Markov Processes with Local Interactions to Networks with a large number of queues, Asymptotical Properties of Queueing ... A.N.Rybko, "Stationary Distributions of Markov Processes Modelling Queueing Networks". ...

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• Conference "Combinatorial Methods in Physics and Knot Theory" (February 2005)
• Semiclassical Microlocal Analysis (Fall 2003)
• Hamiltonian structures and evolution equations (Fall 2001)

... Dave's Universe . ... Scientists release most accurate simulation of the universe to date . A principal purpose of the Bolshoi simulation is to compute and model the revolution of dark matter halos. ... The Bolshoi supercomputer simulation, the most accurate and detailed large cosmological simulation run to date, gives physicists and astronomers a powerful new tool for understanding such cosmic mysteries as galaxy formation, dark matter, and dark energy. ...

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• Astronomy Magazine - Interactive Star Charts, Planets, Meteors, Comets,
• Cosmic giants shed new light on dark matter | Astronomy.com
• Ultracold Big Bang experiment simulates evolution of early universe |

Stellarium 0.12.3 . ... Classes . ... FileљStructure . ... StelToneReproducer Class Reference . ... Set the eye adaptation luminance for the display (and precompute what can be) Usual luminance range is 1-100 cd/m^2 for a CRT screen. ... Set the eye adaptation luminance for the world (and precompute what can be) More... љ . ... Return adapted luminance from world to display. ... Return adapted luminance from world to display with 1 corresponding to full display white. ... xyYToRGB (float *xyY) const . ...

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• Ключевое слово ?Galaxy Evolution Explorer?
• Stellarium: SphereParams Struct Reference
• Stellarium: StelGeometryBuilder Class Reference

... In some cases the plasma is not in the thermal equilibrium, and we need to use the kinetic description. ... A D ) Pa i r p l a s m a M o s c ow , D e c e m b e r 2 0 1 0 27 / 36 Conclusions 1 2 3 We get two types of equilibriums in e , plasma from ...rst principles. 1. kinetic equilibrium with T , 6= 0, timescale (n0 c ) 1 due to 2 particles reactions . 2. thermal equilibrium with T , = 0 due to detailed balance in 3 particles reactions timescale (ne 0 c ) 1 ...

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