... Marshall A.W., Olkin I. - Life Distributions: Structure of Nonparametric, Semiparametric, and Parametric Families . ... Название: Life Distributions: Structure of Nonparametric, Semiparametric, and Parametric Families . Авторы: Marshall A.W., Olkin I. Аннотация: . ... This book includes an extensive discussion of a wide variety of distribution families-nonparametric, semiparametric and parametric-some well known and some not. ...

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• von Davier M., Carstensen C.H. - Multivariate and Mixture Distribution Rasch
• Billinge S.J.L., Thorpe M.F. - Local structure from diffraction :: Электронная
• Von Grudzinski O. - Quasihomogeneous distributions :: Электронная библиотека

... 7 (495) 939-16-82 info@physics.msu.ru . ... Japan), and Univ. of Oulu (Finland) demonstrated that a power-law size distribution with large-size cutoff, as observed in Saturn's rings, is universal for systems where a balance between aggregation and disruptive collisions is steadily sustained. ... We show that a power-law size distribution with large-size cutoff, as observed in Saturn's rings, is universal for systems where a balance between aggregation and disruptive collisions is steadily sustained....

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... Advanced Observation and Modeling of Acoustic Cavitation Structures . R.Mettin, W.Lauterborn, D.Krefting, P.Koch (Drittes Physikalisches Institut, Goettingen University, Goettingen, Germany); J.Appel (Drittes Physikalisches Institut, Goettingen University, Germany) . ... High power input of ultrasound to liquids causes acoustic cavitation. In typical resonator set-ups, the cavitation bubbles form dynamic structures that result in an inhomogeneous bubble distribution. ...

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Twilight observations with MASS/DIMM B. Safonov Sternberg Astronomical Institute Moscow State University Comprehensive Characterization of Astronomical Sites, 2010 B. Safonov (Moscow State University) Twilight observations with MASS/DIMM SITE 2010 1 / 17 Why observe in twilight with MASS/DIMM? ... ASM includes 3 devices sensitive to background: guider, DIMM and MASS. B. Safonov (Moscow State University) Twilight observations with MASS/DIMM SITE 2010 2 / 17 Background in guider. ...

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• Results of recent and ongoing site programs

ASTRONOMICHESKII TSIRKULYAR No.1573, 2010 April 12 1995 2009 . A Comparison of the Latitudinal Variations of the Methane Absorption Bands on Saturn's Disk at Equinoxes 1995 and 2009 Abstract. The observations of Saturn at last equinox 2009 have detected significant differences of the latitudinal variations of the methane absorption from observed at 1995 equinox . ... 1995 . 2008- 2009 , ­ . ... 4 ( 580-880 ) , (.1) , 2008-2009 . ... 2 , 4 725 1995 2009 . ... 1995 2009 15 , 1980 1995 . ...

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Databases (NSDC) of the Natural Planetary Satellites. ... NSDC: Database of astrometric observations of Natural Planetary Satellites . ... They are thoroughly looking for observations in different sources, creating their owndatabases which are then mostly inaccessible to other researchers. ... In the file "content" with explications, the reference is given to the data source as well as the bibliographic reference. ... Data sources. ... Why a specific bibliographic database for Natural satellites? ...

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... We proposed that information retrieved from the local surface photometric behavior of the Moon could be used for guiding the remote sensing analyses of specific geological targets. ... The value of the difference of intensities mentioned above may be used as a photometric parameter I of the local surface roughness. ... 7] Apollo 11 Prelim. ... Figure 5 represents the diagram of relationship between photometric roughness parameter and local thorium content in different lunar regions. ...

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• http://selena.sai.msu.ru/Chik/Publications/Aitken/MS015.pdf
• http://selena.sai.msu.ru/Shev/Publications/ms38/ms083.pdf
• http://selena.sai.msu.ru/Symposium/ant.pdf

... Hydrophobic contacts . ... 28 3D-structures of ETS domain were superimposed by means of SSM server with the following results: . ... H. sapiens . ... By means of CluD the hydrophobic core of every structure was analyzed. ... Totally 41 residues are engaged in the conserved hydrophobic core, 31 of them are at the same time conserved according to Pfam alignment. 21 of those residues do not make any contacts to DNA, thus being important only due to their role in hydrophobic core of the ETS domain. ...

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• ETS_all_contacts alignment
• ETS_water_bridges
• HTH3_3D_conservation

... Algorithm & . Format requirements . ... SDPsite is a tool for identification of protein active and other functional sites, based on spatial clustering of SDPs (specificity-determining positions, described here ) with CPs (conserved positions). ... Mapping predictied positions onto structure and construction of the best cluster . ... The input data of the algorithm are a multiple protein alignment divided into specificity groups . ... is called statistical significance of the set of k* positions . ...

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• SDPpred

... Research objects and scientific purposes . Space scientific program includes development and launch of two supersmall spacecrafts "Universitetskiy" and "Kompas-2" intended for monitoring of radiation conditions near the Earth. ... All the studies conducted in the near-Earth space are characterised by strong radiation fields. ... The circular polar orbits, which cover all the near-Earth space, are the most favorable for comprehensive studies of the radiation conditions near the Earth. ...

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. Subsections . CTEQ4m distribution functions . MRS structure functions . Backscattered photon spectrum . Weizsaecker-Williams approximation . ISR and Beamstrahlung .

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• [Comphep-common] uncertainty on 2l invariant mass distributions of ZZ...
• [Comphep-common] Particle Distribution Functions
• CTEQ4m distribution functions

Next: Where to Get More Up: Sendmail+IDA Previous: Reporting Mail Statistics . ... Accordingly, it is necessary to ensure that all the various pieces of the system (USENET news, mail, TCP/IP) agree on the location of the local mail delivery program (lmail, deliver, etc.), remote mail delivery program (rmail), and the mail transport program (sendmail or smail). ... The following are some problems we've seen in the past with some of the commonly available binary distributions and sources. ...

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• Extracting the binary distribution

... Galaxies rotate and move in clusters as if a tremendous amount of unseen matter is present. But does dark matter exist in the greater universe too -- and if so, where? ... In the above frame from a computer simulation of our universe , a 300 million light-year slice shows dark matter in gray and galaxies as colored circles. ... Publications with keywords: universe - dark matter - 2dF survey - simulation . Publications with words: universe - dark matter - 2dF survey - simulation . ...

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• Journal "Peremennye Zvezdy"
• Астронет > Finding Dark Matter
• Астронет > Archive of Astronomical and Astrophysical Transactions

Measurements of B р Xsl+l- and BрK(*) l+l- at Belle A. Ishikawa (KEK) 18, Aug, 2004 32 nd International Conference on High Energy Physics BICC, Beijing, China Introduction n bрs l+l Е Е Е Е - Е First observed by Belle in BрKll Proceed through penguin, Z penguin and W box diagrams Sensitive to new physics Sign of Wilson coeffient C7 as well as C9 and C10 can be obtained from q2 distribution and AFB(q 2). ... Four background sources Е Е Е Е dilepton events from continuum, mostly from charm events. ...

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• http://nuclphys.sinp.msu.ru/conf/lpp14/210809/Peshekhonov.pdf
• http://nuclphys.sinp.msu.ru/school/s08/s08_13.pdf
• http://nuclphys.sinp.msu.ru/school/s09/09_26.pdf

... J.K. Krylov . In the monography by R. Koehler [1] there was described a very interesting effect of the words' average length oscillation as a function of their frequency of use (according to the data from a representative frequency dictionary). ... In this context, further the Koehler's effect will be definied as polymodal character of the dependence of the conditioned average in cases of two-dimencional distributions of any linguistic nature. ...

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Search for Flavor Changing Neutral Currents in Single Top Quark Production -1 using 2. fb at D 3 Maxim Perfilov Moscow State University on behalf of the D0 Collaboration QFTHEP2010 , 2010 /09/14 Tevatron -396 ns between bunches - - has delivered about 9.2 fb since 2002 1 QFTHEP2010 , 2010 /09/14 2 FCNC models with soliton structure of the top quark Flavor Changing Neutral Currents change flavor of quarks without changing the charge models with ...

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• http://qfthep.sinp.msu.ru/talks/ginzbbdark100912.pdf
• http://qfthep.sinp.msu.ru/talks2013/QFTP-2013_Bodnya__Derkach__Kovalenko__Puchkov__Feofilov1.pdf
• http://qfthep.sinp.msu.ru/talks2013/qfthep_anom_tW.pdf

by Margarita Dzhalalova It is known that the pressure difference values for a round parachute are constant over total canopy, then for a square parachute the values of pressure difference are non-uniform along radial ribbons differing even from each other and depending mainly on certain sets of line lengths, and therefore square parachutes attain different shapes from each other ( Fig.1 - photo of var.1 and var.2). ... Distribution of pressure coefficient along radial ribbons of square parachute. ...

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• Air-Permeability Influence on Pressure Distribution Character

... 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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• APPLICATIONS: Plasma Physics | Moscow University Supercomputing Center

Arshakian T. G., Stepanov R., Beck R., Krause M., Sokoloff D. Simulations of total and polarized emission in evolving galaxies: "spotty" magnetic structures, AN, {\bf 332}, N5, 524-536, 2011 . Magnetic fields in nearby, star-forming galaxies reveal large-scale patterns, as predicted by dynamo models, but also a variety of small-scale structures. ... Ключевые слова: magnetic fields - dynamo - galaxies: magnetic fields - galaxies: high-redshift ...

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• Beck R., Frick P., Stepanov, R., Sokoloff D. Recognizing magnetic structures by
• D.Moss, R.Stepanov, T.G.Arshakian, R. Beck, M.Krause, D.Sokoloff, Multiscale
• Sokoloff D., Zhang H., Moss D., Kleeorin N., Kuzanyan K., Rogachevski I., Gao

... Let $(X_n)$ be a strictly stationary random sequence with the marginal distribution functions $F(x)=P{X_1\leq x}$. ... Let us denote $ M_n=\max {X_1,.. ... The limiting distributions of the random vector $(\tilde{M_n}, M_n)$ and "asymptotic independency" of $\tilde{M_n}$ and $M_n$ are obtained under some condition of weak dependency of random variables from sequence $(X_n)$, which is more restrictive than Leadbetter's $D(u_n)$ condition, and some conditions on the sequence $(\varepsilon_n)$. ...

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• http://new.math.msu.su/department/probab/bsk_28_04.pdf