... High Brightness RTM . ... Fig.1a: 70-MeV pulsed race-track microtron . Many applications require compact, inexpensive and efficient source of electron beam in energy range 10-100 MeV. ... Beam is focused by accelerating structure, which acts as RF quadrupole singlet, quadrupole triplets (12) installed at the even orbits return path and by electromagnet quadrupole singlet (9) installed at common axis. ... Fig.1b: 70-MeV RTM Schematic . ... Energy gain: 4.8 MeV / orbit . Orbits: 14 . ...

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Tsunami source parameters versus earthquake magnitude and depth: Monte Carlo simulation Mikhail Nosov and Anna Bolshakova M.V.Lomonosov Moscow State University, Faculty of Physics, Moscow, Russian Federation (m.a.nosov@mail.ru) European Geosciences Union General Assembly 2011 Vienna | ... Among all possible parameters of a tsunami source we consider only those parameters which can be unambiguously calculated from the vertical component of co-seismic bottom deformations. ...

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... Hartmann Test Using a Screen With Four Holes 2 Hartmann test with four holes screen The theoretical concept of the primary aberrations measurement by four apertures Hartmann test introduced by "Malacara" * and "SalasPeimbert et. al. ... Black curve show the calculated coefficients for phase screens which have 8 modes of Zernike aberrations and red curve show the calculated coefficient for original phase screen. (a) astigmatism 45 (b) astigmatism 090 14 Coma Coma modes of Zernike aberration. ...

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• Methods and instruments to measure/monitor major site properties

... Next Routine] [List of Routines] NAME: ADD_HEADER PURPOSE: addition information from FITS-headers MPFS-frames DESCRIPTION: The function computes the total exposure, mean value zenit distance and modified FITS header CALLING SEQUENCE: Result =ADD_HEADER( headers ) CATEGORY: reduction MPFS-data INPUTS: Headers = String array FITS-headers from the MPFS data OUTPUTS: Header = String array containing the header from the FITS file. ... OPTIONAL INPUT KEYWORD PARAMETERS: BEFORE = Keyword string name. ...

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... 6 4, 53^57, 20 01 The Local Plasma Frequency Approach in Description of the Impact-Parameter Dependence of Energy Loss V. A. Khodyrev* Institute of Nuclear Physics, Moscow State University, Moscow 11989 9, Russia Received October 26, 2 0 0 0; revised ... The local energy loss is determined by the induc ed electron current and the intensity of the projectile ў eld at a given point. ... Fig. 3 shows also the results of calculation of DE b based on the static electron gas model (ek; o from Eq. ...

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• http://danp.sinp.msu.ru/LIIWM/PhysRevA62_2000_022718NMKab.pdf
• http://danp.sinp.msu.ru/LAS/Nimb212_03_96Teplova.pdf
• http://danp.sinp.msu.ru/LIIWM/ArXiv-0904.2151v1_Khodyrev2009.pdf

Заседание 320 (24 октября 2014 г., совместное заседание с семинаром механико-математического факультета 'Современные проблемы математики и механики') . ... B. Emek Abali (Технический Университет Берлина) Thermodynamically modeling of nonlinear rheological materials and a new energy-based approach to determine the corresponding material parameters. A thermodynamical system can be described by the field equations that are governed by the balance equations and the appropriate constitutive equations. ...

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... Boris A. Grishanin is an Associate Professor in the Department of Physics, M.V.Lomonosov Moscow State University (MSU). He received his M.S. and Ph.D. degrees from MSU in 1963 and 1968, respectively (both in Physics). ... B. A.Grishanin's current research interests are in the field of quantum theory of open systems, laser physics, molecular dynamics of photoexcited molecules, problems of quantum information and quantum computing. ... Information theory . ... 2016 Quantum Information Laboratory. ...

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Anisotropy of Cosmic Rays. Origins, experiments, data analysis problems & methods. ... ANTARES problems and methods. ... 2D» experiments Name Tibet Air Shower Array Position 90.522o E, 30.102o N; 4300 m above sea level 30.11 N, 4300m a.s.l. Gran Sasso, 2000m Caucasus, 1700m (40deg N, 113 deg W), atmospheric depth of 860 gm/cm2 Energy 4,6.2,12,50, 300 TeV Gamma /CR mix Time 1997-1999 TibetII, 1999-2001 TibetIII (bigger HD array). 4 years 1 year Statistics 7x109 in ~1000 days Rate Ang. ...

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• http://antares.sinp.msu.ru/docs/INFN%20-%20Paper%203.pdf

... VaST is a software tool for finding variable objects on a series of astronomical images. ... VaST performs object detection and aperture photometry using SExtractor on each image, cross-matches lists of detected stars, performs magnitude calibration with respect to the first (reference) image and constructs a lightcurve for each object. ... VaST FITS image viewer ./pgfv . ... Part I" PZP, vol. ... K. V. Sokolovsky, S. A. Korotkiy; "New Variable Stars Discovered by the NMW Survey" PZP, vol. ...

90. A.V.Shanin

91. Download Yuri Shvarov's files

92. ENSDF Relational

93. http://beams.chem.msu.ru/doc/Dynamical_systems_Theory_and_applications.pdf

94. http://qi.phys.msu.su/papers/2007-prl-99-063901.pdf

95. Scientific Achievements

96. http://library.biophys.msu.ru/PDF/3347.pdf

97. Index of /rus/lab/mol/234/_vti_cnf

98. Kirill A. Kazakov

99. http://nanolab.phys.msu.ru/sites/default/files/romodina_et_al-2015-direct_measurements_of_magnetic_interaction-induced_cross-correlations_of_two.pdf

100. http://herba.msu.ru/shipunov/school/biol_154/2010_2011/lab_03.pdf