... Next: Cheating Poisson: A Up: Statistical Analysis Previous: Spatial Models and . ... The spatial distribution of stars in the Local Group dwarf irregular galaxy NGC 6822 has been studied, using recent positions and deep photometry for about 15,000 stars in the galaxy. Based on photometrical data, OB stars and red stars could be studied separately. Spatial statistical tools have been applied to the analysis of the spatial structure. ... Figure: Model selection by the aid of CAIC . ...

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• Data Models and Formats
• Synthetic Images of the Solar Corona from Octree Representation of 3-D Electron
• Simulation of HST PSFs using Tiny Tim

ASC-FITS-2.0.1: ASC FITS File Designers' Guide (Rots and McDowell) (1999 Jun) . ASC-FITS-REGION-1.0: FITS region document (McDowell and Rots) (1998 Mar) . ... CXC-DM-001 Introduction: Data Analysis with the Chandra Data Model (2001 Oct) . ... 1998 Feb 26: SDS-1.0: Data Product List: obsolete . ... 1998 Mar 09: SDS-10.0: (ASC-FITS-REGION-1.0) FITS region document: see ASC-FITS-REGION-1.0 . 1998 Feb 09: SDS-11.0: FITS function document (superseded by ASC-FITS-FUNCTION-1.2) . ...

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• Jonathan's ASC documents
• Vertical Structure of the Secondary: Hydrostatic Model
• Martin Elvis' Research: Quasar Structure

lte-codes . Sterne . ... In 2006, Behara and Jeffery introduced a new file format for the model atmospheres produced by STERNE and used by SPECTRUM and SFIT. ... allow depth-dependent descriptions of composition, and . ... model.lambda_ref <lambda ref > . ... abundance < elem > < abund > . ... structure.abundance < elem > : ( needs N depth ) . ab elem,1 , ab elem,2 , ..., ab elem,Ndepth > . ... structure.tau_ref : ( needs N depth ) . ... structure.opac_ref : ( needs N depth ) . ...

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• V652HER AND MERGED BINARY WHITE DWARF MODELS
• Chromospheric Modelling
• PhD Thesis abstract

... Buchachenko A.L., Oraevsky V.N., Sorokin V.M., Chmyrev V.M., The model of seismo-ionospheric interaction and its application to the study of ionospheric earthquake precursors with use of alpha station. Abstracts. ... Sorokin V.M., Chmyrev V.M., Sinelnikov V.M., Yaschenko A.K., The physical model underground nuclear explosion and earthquake precursors space monitoring. ... Sorokin V.M., Chmyrev V.M., Yaschenko A.K., Strong DC electric field in the ionosphere related to typhoons and earthquakes. ...

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• SMF2 Ionosphere model Title
• IZMIRAN - Laboratory for Physics and modeling of the ionosphere
• Empirical Model of the Nighttime Winter Ionospheric Trough

The Earth's magnetosphere global structure is conditioned by the interaction of the Solar wind and Earth's magnetic field. ... Many various magnetospheric models are available in the NSSDC . ... Fairfield D. H., Average and unusual location of the Earth's magnetopause and bow shock, J. Geophys. ... Stasiewicz K., Polar Cusp Topology and Position as a Function of Interplanetary Magnetic Field and Magnetic Activity: Comparison of a Model with Viking and other Observations, J. Geophys. ...

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• Lidar homepage - Publications
• Scientific Programme
• Space Research Institute (IKI) Seminar

... Classes . ... Class List . Class Hierarchy . Class Members . include < dustmodel.h > . Collaboration diagram for dust_model: . ... List of all members. dust_pahenhancements . ... dust_carbprops . ... dust_nmoded . ... Represents the entire dust model . 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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• Modelling absorption and emission of radiation by interstellar dust Bojan
• Modelling absorption and emission of radiation by interstellar dust
• Atmospheric Modelling for ALMA Bojan Nikolic web pages (r. 329)

Next: Flagging, Manipulating and Examining Up: Generating Dummy Visibility Data Previous: Making a Fake Observation . If you just want to generate visibilities corresponding to a particular model image, and do not care whether they follow realistic tracks in the uv plane, then im2uv may suit you. Task im2uv simply Fourier transforms an image (whose units should be Jy/pixel) and writes this transform into a visibility dataset. ... IM2UV . ... Normal visibility selection. Only visibilities . ...

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• Multi-Frequency Models
• Modifying Images by Models
• The Structure of Dark Halos: Model-Independent Information from HI Rotation

... G.P.Panasenko (J.-V.Poncelet, Moscow) Multiscale problems: junction of models of different dimension, applications to hemodynamics. ... Gubkina , Moscow, Russia . ... The workshop is devoted to an important trend in mathematical modeling, the multiscale methods and its applications in biology and medicine. ... It was organized in the frame of the thematic year on the multiscale methods and modeling in biology and medicine organized by the Russian-French laboratory J.-V.Poncelet. ...

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• IUM10 conference: A.Belavin, A.Odesskii, R.Usmanov
• The Navier-Stokes-alpha model...
• Conference "Combinatorial Methods in Physics and Knot Theory" (February 2005)

Cost Estimating Web Site . ... 2005 NASA Cost Analysis Symposium Databases . ... World , European Communities , Other European Countries , Americas , Asia , Africa , General US , US Federal Government , US Department of Defense , Aerospace Industry , NASA , Science & Engineering Handbooks . NASA Cost Estimating Handbook 2004 , Parametric Estimating Handbook .. ... Consumer Price Index , Employment Cost Index , GDP Deflator , Import Price Index , NASA New Start Index , Producer Price Index . ...

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. Stellarium 0.12.3 . Main Page . Namespaces . Classes . Coding Style . Scripting . Plugins . Renderer . File Structure . plugins . LogBook . src . models . models Directory Reference . file   . FieldConcatModel.hpp [code] .   . Generated on Sat Aug 10 2013 17:12:46 for Stellarium by   1.8.3.1

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• Stellarium: SatellitesListModel Class Reference
• Stellarium: PropertyBasedTableModel Class Reference
• Stellarium: FieldConcatModel Class Reference

... 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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• Modelling the Milky Way in the Era of Gaia - JD5 programme
• Vladimir P. Reshetnikov's Home Page
• Model of clusters

... Metallic?а nanostructured mesostructures are formed as a result of their self-assembly while growing of nanoclusters and nanowires during the pulsed current electrodeposition process on the membranes. Our work shows that the pulsed current electrodeposition on the templates is a general biomimetic method to fabrication of metal models of natural objects: protozoa, plants, mushrooms, shells. ... тАвThe growth on the?а membranes or templates . ... The layered structure . of the shell . ...

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• Laboratory of materials for electrochemical technologies ISSP RAS
• Spectroscopy of Semiconductors and Dielectrics
• Program - CC-2010, CC 2010, 8th Conference on Cryocrystals and Quantum Crystals

Computer models of objects (galaxies, circumstellar disks, etc.) are often generated to compare with observed images. ... When comparing models to WFPC2 images, it is often forgotten that the instrumental PSF can have a very significant effect. ... Also, the undersampling of the WFPC2 cameras makes the model image very sensitive to subpixel alignment. ... Left) WFPC2 WFC F814W image of HH30 (0.1 arcsec/pixel); (Middle) Model of HH30 disk; (Right) Model of HH30 disk convolved with a Tiny Tim model PSF. ...

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• Retrieving and Archiving SPSS Orbit Model Data
• Modelling
• Comparisons Between Observed and Model PSFs in WFPC Image . Restoration

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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... nonlinear stabilization, the helicity, rotation and small-scale structures influence, the precursors of crisis processes development, the modeling of coherent structures evolution, applications in the natural disasters forecasting, for the helical structures generation in plasmas and astrophysics . ... Large-scale instabilities in hydrodynamics and plasmas . ... The turbulence in plasmas and in the atmosphere and MHD-turbulence . ...

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• Magnetic field models[Oulu]
• REMOTE SENSING OF OCEAN SURFACE STATE
• International Conference "MODE CONVERSION, COHERENT STRUCTURES AND TURBULENCE"

My research interests are focussed on the theory and modelling of accretion processes as well as star and planet formation mechanisms. I am particularly interested in the stability properties of accretion discs, the generation of MHD turbulence and associated angular momentum transport, disk - planet interactions and the origin and characteristics of jets and winds from accreting systems . ... These results have been published in Salmeron & Wardle, 2005, M.N.R.A.S., 361: 45-69. ...

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• Marc White - Astrophysicist - The Australian National University
• Index of /~akarakas/model_data
• Giant Galaxy String Defies Models of How Universe Evolved

... 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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• My report about the Actor Prolog
• IRE RAS. Computational Physics Laboratory.
• Computational Physics Laboratory. IRE RAS.

... In this poster we propose a hypothesis that within fixed assumptions about internal physics (opacity, thermodynamics, nuclear reactions) a strict relation between the surface helium abundance and the entropy of the adiabatic part of the convective zone exists for all solar models. This hypothesis is verified with models under simplified physics (ChristensenґDalsgaard 1988) and with six evolutionary models computed by ChristensenґDalsgaard (1992). ... 1990, ChristensenґDalsgaard 1991). ...

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• http://crydee.sai.msu.ru/ftproot/pub/local/science/publications/hague.94/hague94.ps.gz
• Program of course
• Solar modeling input physics (thermodynamics, opacity, nuclear reactions)

Direct Electron Imaging Using Back Thinned CCD's . ... where, Vim is the maximum radial emission energy of photoelectrons from the cathode (eV), Vs is the cathode to anode voltage (V), k is the spatial frequency (2 p lp/mm), L is the cathode to anode spacing of the proximity focused diode (mm), d is the field-free region thickness(mm), h is the backscattering coefficient, (G/G 0 .) is the ratio of the average EBS gain of the secondary electrons to the primary gain, and W is the CCD pixel pitch (mm). ...

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• Diffuse Model
• Errors in the Steady State and Quasi-SS Models
• THE TEXAS SURVEY: THE PRELIMINARY

... This article is part of the LWN Porting Drivers to 2.6 series . One of the more significant changes in the 2.5 development series is the creation of the integrated device model. The device model was originally intended to make power management tasks easier through the maintenance of a representation of the host system's hardware structure. ... Which devices exist in the system, what power state they are in, what bus they are attached to, and which driver is responsible for them. ...

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• Papers of Vortex project
• GRB follow-up team
• Olga Maryeva homepage