... we show that the comparison between the calculated and observed numbers of the most ``fragile'' (from the point of view of the binary evolution scenario )   galactic binary types (such as X-ray low-mass X-ray binaries (LMXB), cataclysmic variables (CV),   Be-stars   with compact companions, relative number of visible binary radiopulsars   with normal and compact secondary components) impose certain constraints on the feasible initial ... Phenomenological Kick Velocity . ...

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• Initial Distributions of Binary Parameters
• Initial parameters of compact stars
• Parameters of binary compact star evolution

... 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 . ...

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... Supercomputing Technologies in Science, Education and Industry Almanac Series . ... DRIVER: To develop a model of the interstellar hydrogen distribution in the heliosphere. To apply this model for the analysis of experimental data from different spacecraft. ... The results of the simulations of the formation and evolution of molecular clouds can be used as initial conditions for the current star formation in galaxies. ... Research Computing Center (RCC) of Lomonosov Moscow State University . ...

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MSSM Finite-Temperature Higgs Potential for Phase Transition Mikhail Dolgopolov (Samara State University) Dubinin M. (SINP MSU) Rykova E. (SSU) · · · · Introduction Finite-temperature corrections of squarks Thermal evolution and the critical temperature Conclusions Outline [ M. Dolgopolov, M. Dubinin, E. Rykova Threshold corrections to the MSSM finitetemperature Higgs potential. ... 1973 GeV Ilya F. Ginzburg, M. Krawczyk, Symmetries of two Higgs doublet model and CP violation. ...

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• http://qfthep.sinp.msu.ru/talks2013/QFTP-2013_Bodnya__Derkach__Kovalenko__Puchkov__Feofilov1.pdf
• http://qfthep.sinp.msu.ru/talks/qfthep2010_dubinin.pdf
• http://qfthep.sinp.msu.ru/proceedings2015/Quant_Bezuglov.pdf

Электронная библиотека Попечительского совета . ... Engel K.-J., Nagel R. - One-parameter Semigrs for Linear Evolution Equations . ... Название: One-parameter Semigrs for Linear Evolution Equations . Авторы: Engel K.-J., Nagel R. Аннотация: . ... Электронная библиотека попечительского совета мехмата МГУ , 2004-2016 . ...

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• Engel K.-J., Nagel R. - One-Parameter Semigroups for Linear Evolution Equations
• Harvey A.C. (ed.), Proietti T. (ed.) - Readings in Unobserved Components Models
• Appenzeller I. (ed.), Habing H.J. (ed.), L?na P. (ed.) - Evolution of Galaxies

... This study is based on the analysis of melt inclusions in minerals. ... The analysis of glasses from melt inclusions in hawaiites showed no more than 0.07 wt % F and Cl. The low content of H 2 O in the deep fluids is supported by the investigation of a gas phase in melt inclusions. The more evolved plumasitic trachytes inherit the enrichment of melts in CO 2 fluids, which were observed in fluid inclusions. ... Melt inclusions from the agpaitic trachytes and pantellerites also contain CO 2 . ...

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• http://geo.web.ru/conf/alkaline/2009/Kogarko4.htm
• Trusov Sergey's homepage The influence of boundary layer effects on the melt
• The influence of boundary layer effects on the melt inclusions compositions.

... Calculating the Part of the Nonlinearity Parameter for Two Component System . ... The known relation for nonlinearity parameter B/A allows to calculate the pointed quantity if the value of the derivatives of sound velocity u on temperature T and pressure P are known. The dependence of u on T and P for two component mixture can be found from the relation for sound velocity in the mentioned mixture Umix which was derived by the author earlier. ...

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• Abstract (Invited)

THE PARAMETERS INVOLVED IN HAPKE'S MODEL FOR ESTIMATION OF THE COMPOSITION OF THE EJECTA LUNAR TERRAINS. ... In the previous papers we were estimated the surface roughness of the ejecta lunar terrains by means comparison of the local phase function and the average integrated lunar indicatrix. ... The Hapke's theoretical model of the lunar surface reflection. ... For THE PARAMETERS INVOLVED IN HAPKE'S MODEL: S.G. Pugacheva, V.V. Shevchenko a low-albedo lunar surface parameter Bo = 1. ...

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• http://selena.sai.msu.ru/San/Publications/ms38/ms059.pdf
• http://selena.sai.msu.ru/Chik/Publications/Aitken/MS015.pdf
• http://selena.sai.msu.ru/Pug/Publications/m44_70_pugacheva.pdf

Haiqing Xu, Yu Gao, Hongqi Zhang, Takashi Sakurai, Masaoki Hagino, D. Sokoloff, A.Pevtsov, Magnetic helicity of solar active regions as revealed by vector magnetograms and coronal X-ray images, Publ. Astron. ... Japan, 64, 54, 12 pages, 2012. We have used photospheric vector magnetograms of 15 different solar active regions to calculate the current helicity parameter, ?av, and the linear force-free field (LFFF) parameter, ?best, that fits best the observed transverse field. ...

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• D.Moss, R.Stepanov, T.G.Arshakian, R. Beck, M.Krause, D.Sokoloff, Multiscale
• Arshakian T. G., Stepanov R., Beck R., Krause M., Sokoloff D. Simulations of
• Sokoloff D., Zhang H., Moss D., Kleeorin N., Kuzanyan K., Rogachevski I., Gao

NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...

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EPO . EPO (the Evolutionary Parameter Optimizer) is a small evolution strategy library written in C. The user only has to supply a subroutine for target function calculation and the parameter set boundary values, with the rest of the optimization framework being supplied automatically. ... http://telemann.ltt.rwth-aachen.de/epo/ . ... Available Binary Packages: . Debian Package: No . ... User Comments: . ... No graphical user interface) . SAL Home | Numerical Analysis | ...

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• Cosmic factors of evolution of biosphere and geosphere
• SAL- Programming - Tools & Utilities - STL

CALCULATION OF THE PARAMETERS OF MICROSCOPIC OPTICAL POTENTIAL BY ASYNCHRONOUS DIFFERENTIAL EVOLUTION ALGORITHM Zhabitskaya E.I ., Zhabitsky M.V.1 , Zemlyanaya E.V., Lukyanov K.V. Dubna University, Russi, Dubn; Joint Institute for Nuclear Research, LIT, Russia, Dubna ,141980, Joliot-Curie 6 Joint Institute for Nuclear Research, LNP, Russia, Dubna ,141980, Joliot-Curie 6; Rock Flow Dynamics, Russi, Moscow 1 Differential ... J. of Global Optimization 11,1997, Pp. ...

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• http://www.mce.biophys.msu.ru/archive/doc27224/doc.pdf
• http://www.mce.biophys.msu.ru/archive/doc150820/eng.pdf

... Online Services | ... Construct your query and output by sequental openings of needed fields. One output field must be selected (not be blank) at least. ... Query parameters: . Select for output . ... Energy (keV) . ... Y D H M S MS US NS PS FS AS EV KEV MEV or Stable . ... Energy of the ?-ray (keV) . ... Energy parameters of nucleus (B , Alpha energy, N, P separation energy) . ... Neutron separation energy (keV) . Proton separation energy (keV) . ... Excited energy(keV) . ...

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• CDFE => Online services => Chart of nucleus shape and size parameters
• CDFE => Online Services => Nucleus Ground State Parameters
• CDFE => Online services => Chart of Nuclear Quadrupole Deformations

... LanHEP version 3.2.0 (updated on Sep 30, 2015) source gzipped tar archive. ... LanHEP version 3.1.9 (updated on Nov 16, 2014) source gzipped tar archive. ... LanHEP version 3.1.8 (updated on July 21, 2013) source gzipped tar archive. ... LanHEP version 3.1.7 (updated on June 10, 2013) source gzipped tar archive. ... LanHEP version 2.0.7 (updated on May 24, 2002) source (gzipped tar archive) - the command line option '-mOmega' is implemented to produce the model files for micrOmega package. ...

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• Parameter section
• Widths implementation parameters
• Parameterization via decay scheme

... Orthology relat ions were taken from OrthoDB 6 database [1]. ... The ancestral protein reconstruction in each internal tree node of COPG was made using RAXML 7.4.2 on the basis of best COPG protein alignment (selected by AQU A 1.1) containing only co lumns with limited variation (selected using NOISY 1.5.12), the COPG tree (FASTTREE 2.1) corrected by species tree (using TREEFIX [2]) and calculated amino acid replacement matrices (via MODELESTIMATOR 1.1). ... Acids Res., ...

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• http://mccmb.belozersky.msu.ru/2013/abstracts/abstracts/31.pdf
• http://mccmb.belozersky.msu.ru/2015/proceedings/abstracts/26.pdf
• http://mccmb.belozersky.msu.ru/2015/proceedings/abstracts/24.pdf

The Galaxy Disk in Cosmological Context Proceedings IAU Symposium No. ... The presence of exponential bulges and anti-truncated disks has been noticed in many lenticular galaxies. ... Among our findings in unbarred spiral galaxies, only one galaxy, NGC 5533, has a LSB outer disk (Sil'chenko et al. ... In the frame of this model, the Exponential bulges and antitruncated disks 5 inner disk must be more bright and compact than the usual large-scale stellar disks of spiral galaxies are. ...

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• http://sn.sai.msu.ru/~sil/preprints/ar875.pdf
• http://sn.sai.msu.ru/~sil/preprints/bul_eng.pdf
• http://sn.sai.msu.ru/~sil/preprints/al75.pdf

... The Radon transform (also known as the Hough transform) is formulated as a family of line integrals through a two-dimensional function. ... The Radon transform provides us with a simple means of computing the FF plane of the autochirplet transform, by using the Wigner distribution, and arriving at a transform space that tells us basically the same information as the chirplet FF-plane, except that we benefit from the greater resolution of the Wigner distribution. ...

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• SunSoft
• Explanations for solar physics computing page
• ApSA courses

Simulation of life inside Petri dish, where hypothetic unicellular organisms move and reproduce. ... They can't be changed while simulation is in progress Number of cells [1-10] - number of cells in dish at start of simulation Diameter of Petri dish [100-500] - defines the size of Petri dish Cell's lifetime [1-1000] - defines period of cell's life in dish Asexual(sexual) reproduction (on/off) - activates or disables chosen type of reproduction When you press "Submit" button, simulation is launched. ...

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• evolution
• Evolution
• Changeset 11:53672899af16 тАУ Petri Dish

... Next: Index Up: Scanning Probe Microscopy Image Previous: COM-port initialization file format Contents Index . Figure D.1: Parameters of 3D Images . ... Intensity of material emission (Mat. ... material color for diffused light (Mat. ... material reflection color for directed light (Mat. ... material reflection color for reflected light (Mat. ... intensity of directed light (Light Diffuse) . ... Material Shininess) In our case we use the model, where , and this parameter is called Material Color. ...

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• Tuning tab (RAFM mode)
• Actions with obtained files
• It(Z) tab (STM mode), F(Z) tab (AFM mode), D(Z) tab (RAFM mode).

... About lab . ... Online Journal "Computer graphics and multimedia" (in russian) . ... Algorithms for calculating parameters of virtual scenes in computer vision tasks . ...

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• Videocodecs tuning | Graphics and Media Lab