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21. DUST: dust_carbsdpars Struct Reference
. Main Page . Related Pages . Classes . Files . Class List . Class Hierarchy . Class Members . #include < dustmodel.h > . Collaboration diagram for dust_carbsdpars: . [ legend ] . List of all members. dust_lognormalpars . lnd [2] . double . alpha . double . acutlarge . double . beta . double . at . double . C . Carbonaceous grains size-distribution parameters . The documentation for this struct was generated from the following file: . dustmodel.h . Generated on Fri Jul 11 07:32:08 2008 for DUST by 1.5.5
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Ссылки http://www.mrao.cam.ac.uk/~bn204/devman/dust/structdust__carbsdpars.html -- 5.2 Кб -- 11.07.2008
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22. Project 5 - State Program "Condenced Matter Physics"
... The Russian Federation State Program "Physics of Condenced Matter", the "Superconductivity" division , Project code "Generation-2" . ... The multielement josephson structures are known to allow implementation of the unique properties of the Josephson junctions as electromagnetic waves sources with high change rate of generation frequency, working in the millimeter and submillimeter wavelength diapasones. ... Even the optimal type of the junction electrodynamic interconnection isn't chosen. ...
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Ссылки http://www.cplire.ru/html/oxide233/proj5.html -- 7.9 Кб -- 01.09.2005
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23. Parameters of binary compact star evolution
... Figure: Massive binary evolutionary track. ... A short glance to this track is sufficient to understand that there are a lot of evolutionary scenario parameters, which affect different stages of the binary evolution. Fortunately, a very limited number of parameters has effect on the compact binary merging rate. ... The most important (and practically unique) parameter changing the galactic binary NS merging rate is the distribution of an additional (kick) velocity imparted to NS at birth. ...
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Ссылки http://xray.sai.msu.ru/~lipunov/kionewht/node9.html -- 7.2 Кб -- 16.06.2000
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24. POLIMODEL (V1.00) --- April99 --- POLIMODEL (V1.00)
polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...
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Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/impol/polimodel.help.html -- 6.1 Кб -- 06.06.2006
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25. Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/h' F2
... 18-Jan-2010 17:22 . ... Apache/2.2.3 (CentOS) Server at www.wdcb.ru Port 80 ...
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Ссылки http://www.wdcb.ru/stp/data/Images_of_f-plots/TABL/Tables%20of%20different%20Parameters/h'%20F2/ -- 3.9 Кб -- 03.02.2013
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26. http://www.gao.spb.ru/english/as/j2014/presentations/suvorkin.pdf
... Basic Observables: Zero-differenced phase and code ionosphere-free combinations of global GNSS network stations, corrected by P1-C1 satellite code biases (cc2noncc), daily observations with 30 seconds sampling rate Sites coordinates : IGb08 reference frame coordinates and velocities Displacements: solid tides, ocean loading, pole tide loading (IERS 2010) Geometric model : Receivers antennas eccentricities, absolute receiver and ...
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Ссылки http://www.gao.spb.ru/english/as/j2014/presentations/suvorkin.pdf -- 2427.5 Кб -- 30.11.2014
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27. Model realization and some results
... The perceptron structure, on the basis of which the database is built, is defined by a number of the input and output parameters and a required accuracy. ... The output perceptron data are the expansion coefficients of the scattering matrix elements in series of the generalized spherical functions. ... As the cluster structure depends on the generation conditions the expansion coefficients were averaged over 5--7 realizations of the clusters (for N . ... is the coefficient number. ...
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Ссылки http://www.astro.spbu.ru/DOP/A-PERC/PAPER2/node4.html -- 10.8 Кб -- 19.11.2010
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28. CREATE FULLTEXT CONFIGURATION
... CREATE FULLTEXT CONFIGURATION -- create full-text configuration . CREATE FULLTEXT CONFIGURATION cfgname PARSER prsname [ LOCALE localename ] [ AS DEFAULT ]; CREATE FULLTEXT CONFIGURATION cfgname [ { PARSER prsname | ... PARSER . ... LOCALE . ... Create new configuration test with default parser and ru_RU.UTF-8 locale. CREATE FULLTEXT CONFIGURATION test PARSER default LOCALE 'ru_RU.UTF-8'; =# \dF+ test Configuration "public.test" Parser name: "pg_catalog.default" Locale: 'ru_RU.UTF-8' Token | ...
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Ссылки http://www.sai.msu.su/~megera/postgres/fts/doc/sql-fts-createcfg.html -- 10.1 Кб -- 13.04.2008
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29. Data bases of Natural Satellites. Documentation. Structure
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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Ссылки http://lnfm1.sai.msu.ru/neb/nss/DocStructe.htm -- 11.4 Кб -- 18.05.2009
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30. Parabolic flights for achievement zero gravity: flight parameters,
... Space flight . ... Zero Gravity . ... Characteristics of a Complex Flight: . ... Characteristics of the Reduced Gravity (Lunar Gravitation): . ... Characteristics of the Reduced Gravity (Martian Gravitation): . ... Services / Zero Gravity: General description Technical description Flight parameters Photo gallery Price . ...
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Ссылки http://www.atlasaerospace.net/eng/zgrav-polet.htm -- 38.8 Кб -- 09.04.2016
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31. Conference "Combinatorial Methods in Physics and Knot Theory" (February 2005)
... It satisfies the set of WDVV (associativity) equations in canonical variables. The geometric/integrable content of corrections in 1/N is an important, still unresolved, problem. The only way to construct systematically these corrections is to solve the set of loop equations. We find the subleading correction (the torus approximation) and discuss its possible singularities of the answer in the set of new parameters S_i. ...
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Ссылки http://www.mccme.ru/conf_feb_05/chekhov.html -- 2.5 Кб -- 18.02.2005
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32. Astronet > Sky Map, professional edition
... Field size . Object name . ... Map size . ... Field size: the approximate size of the map in the Y direction. ... Galaxies: . ... Galaxies, which size exceeds some value depending on the field and map sizes, are displayed with their real positional angles and sizes by 25m isophote. ... In the "tools" fields there are links to the several famous AVO (Astrophysical Virtual Observatory) resources: NED and Simbad databases and DSS2 (Palomar Digitized Sky Survey) images of the corresponding sky area. ...
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Ссылки http://www.astronet.ru/db/map+/?lang=en -- 30.6 Кб -- 12.02.2011
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33. Department of Solid State Physics MIPT
Chair of solid state physics . ... Laboratory practical training on the structural analysis for 3rd year students of the Solid State Physics Chair of MIPT . ... X-ray diffraction methods in materials research . Debye method: determination of lattice parameters, identification of crystal phases . ... X-ray phase analysis: computer processing of X-ray diffraction spectra, identification of crystal phases using ICDD database . ... X-ray powder diffraction: qualitative phase analysis. ...
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Ссылки http://www.issp.ac.ru/kafedra/en/courses/khasanov.html -- 9.4 Кб -- 28.02.2014
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34. RTT150 Technical Description
RTT150 . ... This optical scheme is similar to 1:7.7 system but has the different parameters of secondary mirror 2 and corrector 3. Primary mirror 1 reflects light to the secondary mirror 2 which collects it on the focal surface of system. Lens corrector 3 is placed between focal surface and the secondary mirror which allows to obtain large flat linear field of 100 mm diameter. Focal length, mm . ... Linear field of view, mm . ... Angular field of view . ... 0.039 mm, %, at least . ...
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Ссылки http://hea.iki.rssi.ru/AZT22/ENG/to_f1173k.htm -- 5.0 Кб -- 18.02.2004
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35. Mikheeva Elena Vladimirovna, Astro Space Center (ASC)
... PhD 1997 in Astrophysics . ... 01 (Theoretical Astrophysics) . ... Astro Space Center . ... Telephone number: . ... FAX number: . ... helen@asc.rssi.ru, helen@lukash.asc.rssi.ru . ... With Daria Kosenko (left) in front of Chateau de Chanonceau (June 2001) . Last modified: 28 June 2007 ...
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Ссылки http://lukash.asc.rssi.ru/people/mikheeva.htm -- 3.1 Кб -- 28.06.2007
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36. . The . MASS . Group .
... Measurement of the MASS detectors parameters with mass program January 24, 2015 [112707] . MASS/DIMM electronics. ... Turbina-core(D): Dimm User Guide. ... N.Shatsky, V.Kornilov, The revision of the MASS/DIMM star catalogue. ... О.Возякова, В.Корнилов, Н.Шатский, Новое программное обеспечение прибора MASS/DIMM. ... V.Kornilov, N.Shatsky, S.Potanin, O.Voziakova, B.Safonov Preliminary results of astroclimate parameters measurements at the Sternberg 2.5m telescope installation site. ...
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Ссылки http://curl.sai.msu.ru/mass/docs.shtml -- 10.3 Кб -- 27.06.2015
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37. COALA - Wolfgang Kerzendor
... Exploring the physics of Type Ia supernovae through spectral analysis . ... Their progenitor scenario as well as the details of the explosion mechanism remain a mystery. ... It produces a supernova spectrum for a given luminosity, photospheric velocity, time since explosion and several elemental abundances. Tweaking these parameters to produce a spectrum that fits an observed spectrum is a complex, as of yet, manual task. ... The search space is large and complex. ...
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Ссылки http://www.mso.anu.edu.au/coala/wolfgang.html -- 4.1 Кб -- 01.10.2012
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38. http://www.ipa.nw.ru/conference/2002/sovet/PS/GAYAZOV.PS
... 8, ``Celestial Mechanics'', 2002 Parameterization of the Solar Radiation Pressure model for GPS satellites I. S. Gayazov Institute of Applied Astronomy, St. Petersburg, Russia The treatment of solar radiation pressure (SRP) effect until now is the main problem in precise modeling of GPS satellite orbits. ... In practice, however, all seven parameters of the empirical model cannot be confidently determined from phase observations. ... BarSever Y. E. A new model for GPS yaw attitude. ...
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Ссылки http://www.ipa.nw.ru/conference/2002/sovet/PS/GAYAZOV.PS -- 29.9 Кб -- 19.08.2002
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39. http://selena.sai.msu.ru/Pug/Publications/m44_70_pugacheva.pdf
THE PHOTOMETRIC RESEARCHS OF THE MERCURY'S SURFACE BY MEANS OF DIGITAL MODELS. ... The surface brightness of Mercury was measured Danjon (1933, 1949, 1953) and Harris (1961) in phase angle 3o-123o. The analysis of the various data of the integral photometric gives the results of determination of the main photometric constants for Mercury. ... THE PHOTOMETRIC RESEARCHS OF THE MERCURY'S SURFACE: S.G. Pugacheva The surface brightness of the Mercurian images was established on the geologic map Mercury. ...
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Ссылки http://selena.sai.msu.ru/Pug/Publications/m44_70_pugacheva.pdf -- 205.0 Кб -- 25.02.2009
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40. East Siberian Center for the Earth's Ionosphere Research. Modelling, secondary
Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Although their determination is based on the scattering process model, independent check-ups by rocket experiments have shown their correctness in experimental applications. ... Ionospheric data analysis, especially during strong disturbances, cannot be without some other kinds of diagnostic tools. ... The lack of data has always been a challange in this case. ...
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Ссылки http://rp.iszf.irk.ru/esceir/isr/ismodelen.htm -- 5.9 Кб -- 04.06.2001
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