Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

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• Restrictions on the Scenario Parameters
• Initial parameters of compact stars
• Initial binary parameters

... 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 => Nucleus Ground State Parameters
• CDFE => Online services => Chart of nucleus shape and size parameters
• CDFE => Online Services => Calculator and Graph Engine for Atomic Nuclei

... 2.5 ISR 63 GeV |y| 2 NA5 19 GeV |y| 1.5 ISR 31 GeV |y| 2 N_ch 2 Regge-Gribov multipomeron approach Probability of production of n pomerons ' ' where n ­ cross section of n cut ... parameters used [1]: [1] Lakomov I. A., Vechernin V. V. , PoS (Baldin ISHEPP XXI) 072 (2012) 4 Regge-Gribov multipomeron approach Mean and variance of the number of pomerons: Variance Mean 5 Description of multiplicity Probability for n strings to give N ch ... Possible solution ­ string interactions. ...

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• http://qfthep.sinp.msu.ru/talks/QFTHEP2010Dolgopolov.pdf

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/Shev/Publications/ms38/ms084.pdf
• http://selena.sai.msu.ru/Pug/Publications/m44_70_pugacheva.pdf

... 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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• COSRAD model - Space monitoring data center

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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Core information (Nucleus, Levels, Gamma transition, Decays, Data type) . ... any adopted (levels and gammas only) experimental . ... Query parameters: . Select for output . ... Levels (E, JPI, T1/2, etc.) ... Energy (keV) . ... Y D H M S MS US NS PS FS AS EV KEV MEV or Stable . ... Energy of the ?-ray (keV) . Relative photon intensity . ... Energy parameters of nucleus (B , Alpha energy, N, P separation energy) . ... Neutron separation energy (keV) . Proton separation energy (keV) . ...

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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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• Moss, D., Sokoloff, D., Lanza, A. F..Polar branches of stellar activity waves:

... 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

const int nvar_ is a number of independent physical parameters involved in the evaluation of squared matrix element. const int nfunc_ is a number of constrained parameters involved in the evaluation of squared matrix element. int calcFunc(void) calculates all constrained parameters for current values of independent ones. It returns 0 in the case of success, otherwise 1. int vinf_(int numvar, char *name, double *val) provides the information about parameters. ... It returns if , or otherwise. ...

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• Widths implementation parameters
• Batch calculations
• Parameterization via decay scheme

... Among the methods of theoretical investigation of coordination compounds, molecular mechanics seems to be an optimal choice. However, conventional MM force fields typically do lack metal-related force field parameters. ... Let us calculate (MM) energy gradient for experimental structures using purely organic force field with no metal-dependent terms. ... In other words, thus calculated forces give an "imprint" for the derivation of metal-dependent forces. ...

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• Solvent effects on exciplex polarity
• Exciplexes of 9-Cyanophenantrene With Electron Donors. Solvent Effect of
• Comparative Analysis of Intramolecular Parameters of Nitrocompounds:

... St