Below are a description of, and links to, the Kurucz (1992) model atmospheres. There are 1100 ASCII files, each containing the fluxes of a Kurucz (1992) LTE model atmosphere. ... The table below gives the available log g values (x 10) and effective temperatures. All models are available for twice solar (p03), solar (p00), quarter solar (m06), and tenth solar metallicity (m10). ... You can find individual files available for FTP on ftp.stsci.edu/science/starburst/Kurucz. ... Solar metallicity . ...

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• Convolving data models with PSF models
• The DIRTY Model. II. Self-consistent Treatment of Dust Heating and Emission in
• Ed Nelan

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(ASC-FITS-REGION-1.0) FITS region document: see ASC-FITS-REGION-1.0 . 1998 Feb 09: SDS-11.0: FITS function document (superseded by ASC-FITS-FUNCTION-1.2) .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
• The AstroStat Slog effective area
• Two-Temperature Raymond Model

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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... По ПЗС-спектрам, полученным с эшелле-спектрометром PFES 6-м телескопа, впервые методом моделей атмосфер определены эффективная температура , ускорение силы тяжести и детальный химический состав слабой звезды, отождествляемой с ИК-источником . IRAS23304+6147. ... Значения эффективной температуры атмосферы объекта, полученные независимо методом моделей атмосфер и путем моделирования распределения энергии в оптическом и инфракрасном диапазонах, совпадают в пределах точности методов. ...

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• Spectral energy distribution

... We present a computer program for modelling energy flux distribution and light curves of eclipsing binaries from far ultraviolet to infrared regions. The Roche model is assumed. Proximity effects of components (reflection of radiation and surface gravity darkening) are taken into account. ... Figure 1: The surface temperature distribution for Algol A-B system before (upper plot) and after (lower plot) correction for temperature due to the irradiation effect. ...

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• Modelling Spectro-photometric Characteristics of Nonradially Pulsating Stars
• A New Entropy Measure Based on Multiple Resolution and Noise Modeling
• Modeling

. This Directory contains Model of distribution of density, temperature and effective collision freguency of electrons. Yu.K.Chasovitin. 1998. This Directory contains The program RIM98 for calculating the parameters of the ionosphere to use the "Reference Ionospheric Model-98" (RIM-98).Yu.K.Chasovitin. 1998.

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• Catalogue 5 of WDC-B

Next: Stellar models Up: Introduction Previous: Photometry Contents . In a hierarchical stellar system, the separation between two neighboring stars is always much smaller than the separation of this pair from the next companion in the system, be it another pair or a single star. ... They are also numerically easier to handle than non-hierarchical systems, since each pair can be described with the standard orbital parameters, and each star with a small number of physical parameters. ... System . ...

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• Stellar models
• ESO - Thesis Topic: Dynamical models of multiple globular cluster populations
• Manipulation of a model

CHANDRA HRMA EFFECTIVE AREA Herman L. Marshall (MIT CXC) CHANDRA HRMA EFFECTIVE AREA Herman L. Marshall (MIT CXC) CHANDRA EFFECTIVE AREA ISSUES HRMA overlayer (with L. David, D. Jerius, etc.) ... 1, 2009 2 HLM-- Chandra Effective Area HRMA AREA MODEL, REVISED Motivation: No overlayer during ground cal (XRCF) Grating XRCF data shows overlayer Cluster kT values disagreed with XMM pn and MOS Pure overlayer models don't fit XRCF data 10 models tried None were perfect Few are very bad One picked: F Apr. ...

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• XMM Radiation Environment Models and Monitor
• Purpose
• Memory Models

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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• FFIT - Command Syntax
• SCL Sfit SLV Commands
• MASSES

The multiscale analysis of heterogeneous structures is actually an important and effective tool of mathematical modeling in physics, technique and biology. ... The special year will extend the existing cooperation between French and Russian researchers in the multiscale analysis and in mathematical modeling in hemodynamics, taking into consideration the mass transport, coagulation, fluid-structure interaction and other aspects. ...

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• The Navier-Stokes-alpha model...
• Sheaf models of linear operators (Spring 2004)
• Theory of finite models (Fall 2001)

Abstract . A self-consistent model for the dynamical and chemical evolution of dense interstellar clouds is examined. The model includes the basic atomic and molecular constituents of dense clouds and the reactions in which they are involved. ... The results of one-dimensional modeling of the early stages of collapse of protostellar clouds of different masses under the action of ultraviolet radiation are presented. Astrophysical applications of the results obtained are discussed. ...

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• chemazh
• Star Formation History

Previous page: Measuring temperatures and composition in the ionoshere . If the actual spectra that the radar measures from the ionosphere consisted of continuous smooth curves, and if it was necessary to measure only two quantities, say the width and the total power, then one could use a ruler and get pretty good answers. ... There is no simple way to get from the data points to the best answers, but one would say that one spectrum is much better than the other. ...

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• ALFA Receiver Temperature Polynomial Fit
• pointing
• Index of /~phil/hardware/12meter/model

... This method is based on putting space modules, vehicles and EVA-suit donned cosmonauts in the swimming pool under conditions of neutral buoyancy, indifferent equilibrium and unsupported state. ... You can also dive into the swimming pool with the SCUBA equipment in order to examine the mock-ups of space stations and vehicles and pass a course of rehabilitation in a hyperbaric oxygenation complex. ... Services / Hydrospace: General description Technical description "Orlan" suit Photo gallery Price . ...

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... To determine the parameters we want (stellar magnitudes and colors) from the observations we have, we fit the data to a model. The model should represent the circumstances of the observations as realistically as possible; otherwise, effects present in the data but not in the model will be distributed among the available adjustable parameters, such as stellar magnitudes, extinction coefficients, and transformation parameters. ... The bias problem . ...

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• Errors in the Steady State and Quasi-SS Models
• Fiber Input Model
• Balloon Model in Java

... FTP access the basic models is here . ... Below, we put short descriptions of the used SED models for the photometric redshifts providing by the current server . ... The uniqueness of this model consists in expanding to the near IR (NIR) of Rocca-Volmerange and Guiderdoni's (1988) atlas of synthetic spectra with a revised stellar library, which includes parameters of cool stars. ... Homepage of the GISSEL model). ... Another model used earlier is the model of synthetic spectra of Poggianti (1997). ...

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... Abstract: We present Monte Carlo radiative transfer simulations for spiral galaxies modelled as a stellar disk and a two-phase clumpy dust distribution. ... As a general result, clumpy models are less opaque than the corresponding homogeneous models. ... 0.00 0.15 0.50 0.1 0.5 1.0 2.0 5.0 10.0 0.25 X . ... We have also produced several homogeneous models, to compare to the clumpy models. ... Homogeneous and clumpy models with the same tauV have the same dust mass. ...

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• Atlas of Monte Carlo Models of Dust Extinction in Galaxies
• Francesco Tribioli - More about my hobbies
• HwB: SGI Mouse (Model 021-0004-002) Connector Connector (Offline)

... Model . ... Karpachev A.T., IZMIRAN, e-mail: karp@izmiran.ru . ... To the Model: . The empirical median model of the shape and position of the MIT (Main Ionospheric Trough) in the Northern and Southern Hemispheres is presented. ... Geomagnetism and aeronomy, v.26, № 1, p.63-68, 1986. ... Karpachev A.T., Afonin V.V. Dependence of the ionospheric trough occurrence probability on the season, local time, longitude, and level of magnetic activity Geomagnetism and aeronomy, v.38, № 3, p.79-91, 1998. ...

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• IZMIRAN: Laboratory for Physics and modeling of the ionosphere - publications -
• IZMIRAN - Laboratory for Physics and modeling of the ionosphere

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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... Towards a Truly Unified Model of AGN . ... The Unified Model holds that the aspect-dependent effects primarily determine the nature of the active galactic nucleus that we observe. ... The full postscript file can be obtained here: . The PASA Latex file can be obtained here: . The postscript file of Fig 1 can be obtained here: . ...

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• Index of /~akarakas/model_data
• Lesson 3: Residual Plots and Chi-Squared Fitting of Models to Data
• Emma Kirby - Science

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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• Folding Paper Model of Magnetosphere
• Folding Paper Model of the Magnetosphere
• Space Research Institute (IKI) Seminar