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http://star.arm.ac.uk/~jgd/chrom_mod.html.
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1. Vertical Structure of the Secondary: Hydrostatic Model
... In this section, we develop a physical model of the secondary as a disk that is centrifugally supported in the radial direction and hydrostatically supported in the vertical direction. We assume that the disk is vertically isothermal and well mixed. ... where is the mean molecular mass of the gas, is the orbital period at the outer edge of the disk in years, and all of the mass of the secondary has been assumed to be concentrated near its center, so the Keplerian approximation is valid. ...
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Ссылки http://hea-www.harvard.edu/~swolk/thesis/node89.html -- 10.7 Кб -- 01.10.2012
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2. The magnetosphere models
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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Ссылки http://www.iki.rssi.ru/vprokhor/descr/msphere.htm -- 5.8 Кб -- 12.05.1999
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/vprokhor/descr/msphere.htm -- 5.8 Кб -- 12.05.1999
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[ Сохраненная копия ] Ссылки http://www.cosmos.ru/vprokhor/descr/msphere.htm -- 5.8 Кб -- 12.05.1999
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3. Spatial Structure of NGC 6822: An Example for Statistical Modeling of
... 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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Ссылки http://www.adass.org/adass/proceedings/adass94/pasztorl2.html -- 11.0 Кб -- 03.11.2000
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4. The DIRTY Model. II. Self-consistent Treatment of Dust Heating and Emission in
In this paper and a companion paper we present the DIRTY model, a Monte Carlo radiative transfer code, self-consistently including dust heating and emission and accounting for the effects of the transient heating of small grains. ... As an illustrative case, we apply the DIRTY radiative transfer code to starburst galaxies wherein the heating sources are derived from stellar evolutionary synthesis models. ...
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Ссылки http://www.stsci.edu/~kgordon/papers/2001ApJ...551..277M.html -- 4.8 Кб -- 21.01.2016
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5. lte-codes: sterne model atmospheres
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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Ссылки http://star.arm.ac.uk/~csj/software_store/guide/help_stn_model.html -- 8.6 Кб -- 15.09.2006
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6. 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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7. Magnetic field models[Oulu]
... The magnetic field of the Earth has been investigated by satellites for several decades now, and enough of it is known to model its average strength and shape during different levels of overall magnetic activity. Presently the most used empirical global magnetic field models are the Tsyganenko models (1987, 1989) , referred to as T87 and T89, respectively, although even these consist of several submodels. ... Earth's magnetic field from T89c model during Kp=2 for different seasons. ... Res. ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/SPPHTEXT/bmodels.html -- 6.4 Кб -- 21.12.2007
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8. XMM Radiation Environment Models and Monitor
. XMM Radiation Environment Models and Monitor . Introduction . Representative Orbits . XMM RM – Geographic Coordinates . Magnetospheric Coordinates (B L) . XMM Data in [B,L] Coordinates . XMM RM – [R, ?] Coordinates . XMM RM Data in L-localtime – No External B Model . XMM RM in L-LocalTime . Solar Proton Contribution . Effects to be Considered . Conclusions . Problems Encountered . Other Points/ Future Activities . Author: Hugh Evans . Email: hevans@estec.esa.nl@estec.esa.nl
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Ссылки http://xmm.vilspa.esa.es/docs/documents/Appendix/HE/index.htm -- 2.8 Кб -- 12.12.2000
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9. Empirical Model of the Nighttime Winter Ionospheric Trough
... Karpachev A.T., IZMIRAN, e-mail: karp@izmiran.ru . ... 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, ? ... 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, ? ... Karpachev A.T. Characteristics of a Ring Ionospheric Trough. ...
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Ссылки http://www.izmiran.rssi.ru/ionosphere/sm-mit/?LANG=ru -- 13.8 Кб -- 09.04.2016
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10. Index of /~akarakas/model_data
... reference to the following paper: Karakas Lattanzio (2007, PASA, submitted) Each file contains: 1) pulse number 2) the core mass , Mcore ( Msun ) 3) maximum mass of the intershell convection zone, M_csh ( Msun ) 4) duration of intershell convection , t_csh (years) 5) mass dredged into the envelope, D_dredge ( Msun ) 6) lambda 7) lambda_dup defined by Goriely Mowlavi (= lambda x (DMh/Mpulse) where Mpulse is the maximum ...
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Ссылки http://www.mso.anu.edu.au/~akarakas/model_data/ -- 3.4 Кб -- 01.10.2012
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11. http://www.eso.org/~rsiebenm/FTP/PPT/Kreta.pdf
AGN dust model of 3CR sources Frank Heymann (PhD), Martin Haas, Endrik Krgel, Christian Leipski MIR imaging spectroscopy ISM dust model PAH SED of a clumpy AGN torus CenA (ESO) Crete 2010 vectorized Monte Carlo model Ralf Siebenmorgen 1) Ground based MIR imaging Nuclear activity in nearby galaxies Surface brightness AGN viz. starbursts Ralf Siebenmorgen 10m telescopes ... Ralf Siebenmorgen Crete 2010 PAH in a mono-energetic heating bath if | ... Crete 2010 ...
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Ссылки http://www.eso.org/~rsiebenm/FTP/PPT/Kreta.pdf -- 1347.3 Кб -- 24.09.2010
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12. Errors in the Steady State and Quasi-SS Models
The Steady State model of the Universe was proposed in 1948 by Bondi and Gold and by Hoyle. ... At the time the Steady State model was proposed, the Big Bang model was in trouble because the value of the Hubble constant was clearly bigger than the inverse of the age of the Universe. ... Thus the Steady State model has flat spatial sections like the critical density Big Bang model. ... The Steady State model has no adjustable parameters to correct for this error, but the Big Bang does. ...
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Ссылки http://www.sao.ru/cats/~satr/cosmo/stdystat.htm -- 7.6 Кб -- 24.10.2000
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13. Meade Instruments Corporation - Meade Model 9200 Microscope Instruction Manual
... Meade Instruments Corporation . ... Microscope Instruction Manual . Meade Model 9200 . ... In any microscope, the objective lens magnifies the illuminated specimen on the microscope Stage, and then is further magnified by the microscope's eyepiece. ... In the case of the Meade Model 9200, use the 4X Objective Lens (6) by rotating the Objective Lens Turret (9) so that the 4X Objective Lens is aiming at the center of the Stage (when it is in the proper position it will click into place). ...
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Ссылки http://www.meade.com/manuals/9200/index.html -- 12.0 Кб -- 10.11.2012
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14. The Structure of Dark Halos: Model-Independent Information from HI Rotation
... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Information & tools for observers . ... Observers archives tools & information . ... Next Section: Fitting Rotation Curves: Mass . ... Although the approximately flat rotation curves of gas in the outskirts of spirals is generally taken as strong evidence for spherical, isothermal dark matter halos, this conclusion is often incorrect and always model-dependent. ... Fitting Rotation Curves: Mass Models Kinematics ....
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Ссылки http://www.atnf.csiro.au/pasa/14_1/sackett/paper/index.html -- 50.7 Кб -- 08.04.2016
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15. Special Year in Multiscale Mathematical Modeling in Biology and Medicine
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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Ссылки http://www.mccme.ru/lifr/medicine.htm -- 3.1 Кб -- 10.09.2014
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16. 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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17. Bojan Nikolic -- Fitting and Comparison of Models of Radio Spectra
... Bojan Nikolic web pages home . Next: Fitting of models of radio spectra --.. ... I describe an approach to fitting and comparison of radio spectra based . on Bayesian analysis and realised using a new implementation of the . ... used maximum-likelihood fitting of radio spectra by allowing objective . ... implementation details of the computer code. ... overall approach described here may also be useful for analysis of other . ... Copyright 2012, Bojan Nikolic feedback welcome ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/blog/2009/12/fitting-and-comparison-of-models-of.html -- 5.5 Кб -- 22.11.2012
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18. NASA JSC Cost Estimating and Models Web Site
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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Ссылки http://www.jsc.nasa.gov/bu2/ -- 15.7 Кб -- 26.11.2004
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19. Atlas of Monte Carlo Models of Dust Extinction in Galaxies
... Abstract: We present an extensive study of the radiative transfer in dusty galaxies based on Monte Carlo simulations. ... We have explored the dependence of A_l on a conspicuous set of quantities (Hubble type, inclination, dust optical thickness, dust distribution and extinction properties) for a large wavelength interval, ranging from 1250A to the K band, thus finally providing a comprehensive atlas of dust extinction in galaxies, which is electronically available. ... S04_MD20[ att , abs ] . ...
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Ссылки http://www.arcetri.astro.it/~sbianchi/attenuation.html -- 9.1 Кб -- 29.03.2002
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20. LWN: Driver porting: Device model overview
... 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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Ссылки http://mavr.sao.ru/hq/sts/linux/doc/porting_to_26/31185.html -- 16.4 Кб -- 28.12.2007
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[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/sts/linux/doc/porting_to_26/31185.html -- 16.4 Кб -- 02.10.2012
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