... Usually runs in the end of a calibration period are acceptable · GroupID format is YYGG.S ­ a float, YY ­ year {8,10}, GGgroup {1,99}, S ­ subgroup {1,} (possibly YYGG.S.S) Example of a group Group 1001.1.1 - 3N+ 2T3 (+GC) Fit and distance 2010 III I II Line reconnections I. 14/11/2009 ­ 11/09/2010, 10 lines 3N+ 2T3 , 1001.1, 187316 min (130 days ) 1/2 gain , 1001.2, 14231 min (10 days ) 1/4 gain , 1001.3, 34230 min (24 days ) 1/8 ... For preliminary and problematic runs. ...

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Documentation on Firefly v. 8.0.0 numerical gradient features . The numerical gradient code is activated as follows: . ... The primary purpose of this code is to allow computations normally requiring analytic energy gradients, to be performed using those QC methods for which analytic gradients are not yet programmed. ... The numerical gradients code is tightly integrated into Firefly and can be used anywhere where the analytical energy gradients are required by default. ... The default is 2. ...

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Geology at Moscow State University . Departments . ... Geology and geochemistry of ore deposits . ... Mineralogy . ... research institutes, and other organizations.The researchers are conducted by the members of several scientific groups which deal with diamond deposits , mineralogy and genetic crystal chemistry of rare elements, experimental thermodynamics and thermochemistry of minerals , genetic mineralogy , spectroscopy of minerals , and mineralogy of porphyry-copper deposits ...

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... 20 , 2014, , Outlines · Cosmological impact of new stable particles: direct and indirect searches for dark matter · Cosmological patterns of particle symmetry breaking: archioles, massive PBH clusters, antimatter domains . ... They are: · Inflation · Baryosynthesis · Dark matter/energy All these phenomena imply extension of the Standard Model of Strong (QCD) and Electroweak Interactions. ... Dark Matter from Charged Particles? ... Advances in High Energy Physics, vol. ...

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... Formulation of the problem ­ angle about the mass center C IC = mR 2 ­ central moment of inertia m and R ­ mass and radius of the hula-hoop k ­ coefficient of viscous friction r ­ radius of the waist FT ­ friction force N ­ reaction force ­ angle between x and CO x = a sin t , IC m m Ё +k (R - (R - y = b cos t = -FT R r ) = m (x sin + y cos ) + FT Ё Ё Ё r ) 2 = m (x cos - y sin ) + N Ё Ё (R - r ) = R ­ non-slippage where constants 0 mod 2 are defined from + µ cos 0 = 0. ...

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Lectures on Nanomagnetism Prof. M. Farle www.unidue.de/agfarle University DuisburgEssen ( Lectures will be given in English with (partial) Russian translation upon request) th Lecture Hall: library of faculty of physics, 5 floor Monday, 24.03.2014 Duration 30 min 15:15 15:45 30 min 15:45 16:15 30 min 16:15 16:45 break 45 min 17:00 ­ 17:45 45 min 17:45 ­ 18:30 Tuesday, 25.03.2014 45 min 15:15 ­ 16:00 45 min 16:00 ­ 16:45 break 45 ...

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... Bohm limit DB=vrg/3: Emax Emax ush 0.3 Ze B Rsh c 1014(B/Bism) Z eV B Hillas criterion ! ... Voelk 2000; Kang Jones 2006) - Bohm diffusion in amplified magnetic field B2/8 = 0.035 u2/2 ( Voelk et al. 2005 empirical; Bell 2004 , Zirakashvili VP 2008 theoretical) - account for Alfvenic drift w = u + Va upstream and downstream - relative SNR rates: SN Ia : IIP : Ib/c : IIb = 0.32 : 0.44 : 0.22 : 0.02 Chevalier 2004 , Leaman 2008, Smart et al 2004, Berezinsky et al 2006 Das et al. ...

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... In later sections, we shall see how seemingly unrelated discoveries in fundamental physics led to a theory of nuclear energy generation in stars that resolved the controversy over the age of the sun and explained the origin of solar radiation. In the section just before the summary, we shall discuss how experiments that were designed to test the theory of nuclear energy generation in stars revealed a new mystery, the Mystery of the Missing Neutrinos. I. THE AGE OF THE SUN How old is the sun? ...

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... UHECR SINP MSU . ... News . ... TUS Ultra high energy cosmic ray detector on-board the Lomonosov satellite . ... According to existing estimations it can be a prominent source of ultra high energy cosmic rays (UHECR). ... In either case, the newly born magnetar is an attractive site for producing ultrahigh-energy cosmic rays (particles with individual energies exceeding 10 18 e V ; UHECRs). ... A new mechanism for the acceleration of ultra high energy cosmic rays (UHECR) is presented here. ...

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131. SAI OCL Catalog Description

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136. http://mph.cs.msu.ru/mph/arh/blank/1999pro-en.doc

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