Lib-DVM - детальный дизайн (оглавление) . Часть 1 . ... 12.16 Запрос и освобождение памяти . RTS err 200.000: no memo ry . ... RTS err 200.001: invalid calloc parameters . ... RTS err 200.002: no memory . ... RTS err 200.003: no memory . ... RTS err 200.004: inva lid malloc parameter . ... RTS err 200.005: no memory . ... RTS err 200.006: no memory . ... RTS err 200.007: invalid realloc parameters . ... RTS err 200.008: no memory . ... 12.18 Средства внутреннего самоконтроля . ...

Еще в разделе: (Показать все результаты (>104) - sp.cs.msu.ru/ )

• Lib-DVM library. Detailed design. Part 3 (12.16-12.18)
• Lib-DVM. Detailed design

... Class . ... public class Schema . ... This is a set of ProtoVariable, the DimensionSet which is the union of the Dimensions used, and any global Attributes. ... contains (java.lang.String name) . ... Returns the set of attributes associated with this, also know as the "global" attributes. ... a new Array containing the elements of this set. public ProtoVariable get (java.lang.String name) . ... If a different ProtoVariable with the same name, was in the set, it is returned, otherwise null is...

Еще в разделе: (Показать все результаты (>82) - angel.cs.msu.su/ )

• : Class AbstractNetcdf
• FileUtils
• : Class ProtoVariable

New achievements in Development of Multidimensional Data Acquisition, Processing and Visualization DAQPROVIS M. MorhА *, 1, 2 , V. Matousek 1, 2 1, 3 , J. Kliman 1, 2 , 1 Institute of Physics, Slovak Academy of Sciences, Bratislava, Slovakia 2 Flerov Laboratory of Nuclear Reactions, JINR, Dubna, Russia 3 Laboratory of High Energies, JINR, Dubna, Russia * E-mail: morhac@savba.sk ACAT - 2002 I. Turzo c 1, 3 , . ... The channels are displayed as balls. ... Four-parameter experimental spectrum. ...

Еще в разделе: (Показать все результаты (>44) - acat02.sinp.msu.ru/ )

... JETP Letters, 57,768(1993)] B (90% CL) 75 kg silicon multi- detector , 600 Si(Li) cells, -flux of ~ 2в1013 / cm 2 / s , 30 days on /17 days off 1 .9 в 10 ­10 B (95% CL) 6 upper bounds upper limit Solar SK+KamLand White dwarfs Red giants Supernova 1987A ... -11 -10 -10 Comments 1.1*10 3*10 3*10 model dependent should not be violated by more than two neutrino species 1.5 *10 5.4*10 7.2*10 9*10 -11 -11 -11 7 measurement under ... Advances in High Energy Physics. ...

Еще в разделе: (Показать все результаты (>163) - nuclphys.sinp.msu.ru/ )

• http://nuclphys.sinp.msu.ru/mirrors/1998_8.pdf
• http://nuclphys.sinp.msu.ru/school/s09/09_02.pdf
• http://nuclphys.sinp.msu.ru/conf/lpp14/220809/Demidov.pdf

Chiral symmetry and form factors of neutrino-nucleon interactions. Kanshin Kirill Vereshkov Grigory Southern Federal University, Russia QFTHEP '11, Sochi 24th Sept.­ 1st Oct. ... The united theory of leptonnucleon interactions · Neutrino Charged Currents · Neutrino Neutral Currents Kanshin K., Vereshkov G. Southern Federal University, Russia Page 2 Chiral symmetry and form factors of neutrino-nucleon interactions. ... It is based on meson dominance and chiral symmetry of strong interactions. ...

Еще в разделе: (Показать все результаты (>170) - qfthep.sinp.msu.ru/ )

• http://qfthep.sinp.msu.ru/talks/qfthep2010_dubinin.pdf
• http://qfthep.sinp.msu.ru/talks2013/QFTP-2013_Bodnya__Derkach__Kovalenko__Puchkov__Feofilov1.pdf
• http://qfthep.sinp.msu.ru/talks/QFTHEP2010Dolgopolov.pdf

... Page 2 NEMO Numerical modelling Page 3 · Ocean in equations y (Approximations of) Equations of geophysical fluids x Coherence and extrapolation: · spatial (« representation of a 3D fiel · temporal (« keep in memory... and ... forecast ») ds ») · inter-variables (« measure temperature, deduce salinity, compute currents...») z (t) (t+1) Integrated system Page 4 SATELLITE observation s SSALTO MODELISATION ASSIMILATION IN SITU ...

Еще в разделе: (Показать все результаты (>1359) - www.sevin.ru/ )

• http://www.sevin.ru/ecosys_services/references/Puzachenko_Landscape%20as_Dinamic_systems.pdf
• http://www.sevin.ru/seminars/argos/Argos%20location.pdf
• http://www.sevin.ru/dissertations/submitted/2015_Olchev/references_2.doc

... Data . ... Services . ... Solar energetic particles . ... N -d SW Conditions : Time profiles of the key geomagnetic ( Ap and Dst indices), solar wind (velocity V , density n and temperature T ) and IMF ( B , Bx , By , Bz in GSM) parameters observed in the N day vicinity of the geomagnetic disturbed day. N -d Map of Solar Events : Map of solar surface events occurred within N day vicinity of the moment when the solar wind expansion (which causes the geomagnetic event) started. ... WIND . ...

Еще в разделе: (Показать все результаты (>40) - smdc.sinp.msu.ru/ )

• Space monitoring data center
• COSRAD model - Space monitoring data center
• Paraboloid model of the Earth's magnetosphere - Space monitoring data center

The purpose of the space-physics lab exercises is to introduce the students to the methods of the measurements, to the modern conception of near-Earth space structure and the physical processes and phenomena occured in it. ... At present the reasearches and the teachers of the University and of other institutes participating in the project continue development of the the special space-physics lab exercises, and they are interested in your ideas concerning the future exercises. ...

Еще в разделе: (Показать все результаты (>6731) - cosmos.msu.ru/ )

• University Satellites and Space Science Education '2006
• University Satellites and Space Science Education '2006 I

diploma thesis abstract of Zjabko I.A. Anisotropy of a parameter of absorption in thin films of polymer polyparaphenilvenylene and donor-acceptor compositions on its basis In the present work are investigated thin a film of the connected polymer of a soluble derivative polyparaphenilvenylene (PPV). ... The received experimental curves are approximated by theoretical dependence and thus required values of optical constants are determined. ...

Еще в разделе: (Показать все результаты (>76) - ofvp.phys.msu.ru/ )

• http://ofvp.phys.msu.ru/en/science_education/diploma/annot/2011/Trukhanov_Bruevich_en.pdf
• http://ofvp.phys.msu.ru/en/science_education/diploma/annot/2015/Yakovlev_Zapunidy_en.pdf
• http://ofvp.phys.msu.ru/en/science_education/diploma/annot/2013/Genkin_Saveliev_en.pdf

The QKeyEvent class contains parameters that describe a key event. ... QKeyEvent  ( int type, int key, int ascii, int state )  . ... void  accept  ()  . ... Key events occur when a key is pressed or released when a widget has keyboard input focus. A key event contains a special accept flag which tells whether the receiver wants the key. ... Constructs a key event object. ... Sets the accept flag of the key event object. ... Clears the accept flag parameter of the key event object. ...

Еще в разделе: (Показать все результаты (>269) - rtm-cs.sinp.msu.ru/ )

• Qt Toolkit - QChildEvent Class
• Qt Toolkit - QMouseEvent Class
• Qt Toolkit - QFocusEvent Class

... The Influence of Microstructure of Media on Nonlinear Acoustic Parameter of Solutions . ... The acoustic nonlinear parameter B/A is strongly structure sensitive as it was shown in [Lesnyanskii et al. ... The values of parameters (Ye/Yid and derivative Ye with respect to pressure) are calculated from offered method [Balankina E.S. Proceeding of XI Session of the Russian Acoustic Society, Moscow, 2001 (http://www.akin.ru/RAO/sess11)] using volumetric-elastic properties of solutions. ...

Еще в разделе: (Показать все результаты (>182) - acs366.phys.msu.su/ )

• Abstract (Invited)

... Structure of Data . ... Catalog . ... In SAI OCL Catalog, we introduce our work on investigation of the Milky Way system of open star clusters. The main goal of our study is a search for new clusters using huge surveys. 168 new clusters have been already discovered by us using J,H,Ks data from 2MASS point source catalog. ... For 141 new clusters, we found their physical parameters using J,H,Ks data from 2MASS catalog and, for a number of clusters, our UBVRI CCD observational magnitudes. ...

Еще в разделе: (Показать все результаты (>20) - ocl.sai.msu.ru/ )

• SAI OCL Catalog Structure

... Let the control system be given by the equation dx = X (x, u) = X, u U, dt where X is a vector field on the configuration space M , x M , u is the control parameter, U is the set of admissible values of u. With the vector field X we canonically associate a scalar-valued fiberwise linear function HX on the cotangent bundle T M , HX ( , u) = , X ( , u) , T M , u U, where : T M - M is the canonical pro jection. ...

Еще в разделе: (Показать все результаты (>16) - pont2008.cmc.msu.ru/ )

• http://pont2008.cs.msu.ru/files/en/abstracts/Krener.pdf
• http://pont2008.cs.msu.ru/files/en/abstracts/Agrachev.pdf

Кафедра ТЕОРИИ ВЕРОЯТНОСТЕЙ БОЛЬШОЙ СЕМИНАР КАФЕДРЫ ТЕОРИИ ВЕРОЯТНОСТЕЙ (руководитель - член-корр. РАН, профессор А.Н. Ширяев) February 9 - An approach to calculating the variance of Pitman estimators Alexander Novikov (University of Technology, Sydney) Nino Kordzakhia (Macquarie University, Sydney) We provide an analytic formula for the variance of the Pitman estimator for a location parameter of independent observations and also some change- point estimators. ...

Еще в разделе: (Показать все результаты (>40) - new.math.msu.su/ )

• http://new.math.msu.su/department/probab/bsk_28_04.pdf
• Andrei Vladimirovich Fursikov | Department: General Problems of Control.

О лаборатории . ... Лаборатория теоретической биофизики . ... Here the guide to use RESP technique based on calculations from Firefly or GAMESS-US is presented. ... Note, that RESP algorythm will fit potential in the set of points which are selected according to $PDC group in the input-file. ... Нет комментариев " Using RESP with GAMESS-US and Firefly (PC-GAMESS) " . ... Using Firefly/GAMESS-US efficiently . ... Scannin? in Using Firefly/GAMESS-US efficiently? 2012 ERG Research Group . ...

Еще в разделе: (Показать все результаты (>13) - erg.biophys.msu.ru/ )

• gromacs ERG Research Group: Лаборатория теоретической биофизики

M.H. Shulman, 2006 Michael H. Shulman ON AN IMPORTANT COSMOLOGICAL PROBLEMS SOLUTION IN THE FRAME OF A NEW COSMOLOGICAL MODEL Abstract A modification of the Einstein ­ Friedmann cosmological model allows to solve a basic cosmological fundamental and observational problems, such as these ones: the vacuum energy and dark energy problems, horizon problem, flatness problem, supernovae low brightness at the high redshift (z > 1). ... New cosmological model The upper curve on the figure 2 is linear. ...

Еще в разделе: (Показать все результаты (>369) - chronos.msu.ru/ )

• O.S.Razumovsky. Models of Time in Physics and Cosmology
• Шпенков Г.П. (G. P. Shpenkov)
• Крейдик Л.Г. (L. G. Kreidik)

log . ... Sat, 26 Mar 2011 02:18:36 +0300 . boris (kodomo) . ... Daniil Alexeyevsky . ... Typo in allpy.fileio.write_strings . ... Fri, 25 Mar 2011 23:12:21 +0300 . ... Automated merge with ssh://kodomo/allpy . Thu, 17 Mar 2011 17:48:37 +0300 . ... Wed, 16 Mar 2011 22:50:50 +0300 . ... Mon, 28 Feb 2011 22:40:16 +0300 . ... allpy.processors: make temporary files named . Tue, 01 Mar 2011 00:17:13 +0300 . boris . ... Updated allpy/data/codes.py from fresh components.cif . ...

Еще в разделе: (Показать все результаты (>5240) - kodomo.fbb.msu.ru/ )

• allpy: 1785e40b2a2d .hgignore
• allpy: 1785e40b2a2d .hgtags
• allpy: 1785e40b2a2d test/test.py

'mpif.h' * Именованные константы - параметры задачи INTEGER DLEN_, IA, JA, IB, JB, M, N, MB, NB, RSRC, $ CSRC, MXLLDA, MXLLDB, NRHS , NBRHS, NOUT , $ MXLOCR, MXLOCC, MXRHSC PARAMETER ( DLEN_ = 9, IA = 1, JA = 1, IB = 1, JB = 1, $ M = 9, N = 9, MB = 2, NB = 2, RSRC = 0, $ CSRC = 0, MXLLDA = 5, MXLLDB = 5, NRHS = 1, $ NBRHS = 1, NOUT = 6, MXLOCR = 5, MXLOCC = 4, $ MXRHSC = 1 ) DOUBLE PRECISION ONE PARAMETER ( ONE = 1.0D+0 ) * * Локальные переменные INTEGER ICTXT , ...

Еще в разделе: (Показать все результаты (>656) - num-anal.srcc.msu.ru/ )

• http://num-anal.srcc.msu.su/eng_math/redict/20.htm
• http://num-anal.srcc.msu.su/meth_mat/parl_prg/pr2_3.htm
• Конвертер с Фортрана на Паскаль

Preliminary results of astroclimate parameters measurements at the Sternberg 2.5m telescope installation site V.Kornilov, N.Shatsky, S.Potanin, O.Voziakova, B.Safonov Moscow, 2008 Acknowledgements A.Belinskiy M.Kornilov A.Tokovinin M.Kuznetsov P.Kortunov E.Gorbovskoy SAI administration some SAI students Pulkovo solar station (KHSS) staff RFBR support MAVEG Gmbh Why to study optical turbulence and some other relevant ... Mean seeing by DIMM data for this night is 1''5. ...

Еще в разделе: (Показать все результаты (>23) - curl.sai.msu.ru/ )

• . The . MASS . Group .

DESCRIPTION OF THE TIME PROFILES OF KEY GEOMAGNETIC AND SOLAR WIND PARAMETERS . Time profiles of key geomagnetic parameters ( Ap and Dst indices) are shown together with key parameters of the solar wind (velocity V , density n and temperature T ) and IMF ( B , Bx , By , Bz in GSM coordinate system). ... High time resolution data on the solar wind plasma is obtained from Wind experiment in 1997 and ACE experiment in 1998-2002 using ISTP data base . ...

Еще в разделе: (Показать все результаты (>25) - dbserv.sinp.msu.ru/ )

• Catalogue of Space Storms