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(ASC-FITS-REGION-1.0) FITS region document: see ASC-FITS-REGION-1.0 . 1998 Feb 09: SDS-11.0: FITS function document (superseded by ASC-FITS-FUNCTION-1.2) .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 model
• The AstroStat Slog Blog Archive [MADS] multiscale modeling

... 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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• Folding Paper Model of Magnetosphere

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
• Corrected Geomagnetic Coordinates

... 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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• Bojan Nikolic -- Nested sampling modelling of Star-Formation History of the
• Bojan Nikolic -- Fitting of models of radio spectra -- talk at NRAO/Green Bank
• Modelling absorption and emission of radiation by interstellar dust Bojan

... Previous: Algorithms . ... On Fractal Modeling in Astrophysics: The Effect of Lacunarity on the Convergence of Algorithms for Scaling Exponents. ... Using Massively Parallel Processing of a NLTE Spectrum Synthetic Code and an Automated Comparison with Observations to Determine the Properties of Type Ia Supernovae from their Late Time Spectra. ... Copyright 1997 Astronomical Society of the Pacific , 390 Ashton Avenue, San Francisco, California 94112, USA . ...

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• Spatial Structure of NGC 6822: An Example for Statistical Modeling of
• Modelling Spectro-photometric Characteristics of Eclipsing Binaries
• A Method to Test the Adequacy of a Model to Observations

... Modelling is the only feasible way of assessing the reliability of the reconstructions. Modelling here refers to the model used to generate a simulated data set, not the implicit modelling performed by the deconvolution algorithms.) ... Model-fit for parameters to the original data if possible. Check that simulated observations can recover the significant features of the model reliably. ... Use simulated observations to determine the effective resolution of the deconvolution sky model. ...

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• Convolving data models with PSF models
• Prior Models
• Frontier Fields Lensing Models

Next: C.S. Jeffery Up: J.G. Doyle Previous: Magnetic Reconnection Contents . We present, for the first time, blinker phenomena associated with brightenings in pre-existing coronal loops registered by the EIT in Fe XII 195?. ... We suggest that the blinker activity we observe is triggered by interchange reconnection, serving to provide topological connectivity between newly emerging flux and pre-existing flux. ...

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• EVOLUTION MODELS
• Armagh Observatory
• MASSES

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . Mopra radio telescope . ... Australia Telescope Online Archive (ATOA) . ... Australia Telescope 20GHz Survey . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... Probing ISM Models with H observations . ... Turbulent Models of the ISM . ...

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• Self-Calibrating with Multiple Models
• Generating Visibilities from a Model Image
• MODELS tasks

... 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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• SMF2 Ionosphere model Title
• Magnetism ADB

... 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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• Diffuse Model
• Errors in the Steady State and Quasi-SS Models
• Reducing the observations

... Comparing the periods from the model and P2030 data (.ps) ( .pdf ) . aeroPer.dat...file containing aerostat periods. ... The model was then used to determine the periods that it could generate in pulsar observations. ... rf pulse length: 320 Useconds (this is actually 2 160 usecond pulses that are sequential in time). 7 ipps of 3771., 3504., 3076, 2809., 2903.5, 3289., and 3676. useconds. blanking of the radar signal for 42 degrees of azimuth centered on the observatory direction. ...

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• Modeling the Spectrum
• Index of /~phil/hardware/12meter/model
• Figures for Scattering Paper

... The most powerful and widely used methods to calculate the scattering matrix of a fractal cluster are based on the coupled dipoles methods (e.g. the Discrete Dipole Approximation, DDA) and the theory of light scattering by a cluster of spherical particles [2-4]. ... At present the procedure of calculation of the scattering matrix is well developed for both an oriented cluster of spherical particles and for chaotically oriented clusters of such particles [4]. ...

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• Model realization and some results
• Modelling the Milky Way in the Era of Gaia - JD5 Rationale
• Modelling the Milky Way in the Era of Gaia - JD5 programme

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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Refinements on precession, Nutation , and Wobble of the Earth VИronique Dehant, Royal Observatory of Belgium ROB rigid Earth nutation Forced Nutations oceanic/atmospheric corrections Non-rigid Earth nutation model Earth response comparison with observation Earth interior model ROB Earth rotation changes due to the core ; core - mantle coupling coupling mechanisms: topographic ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/filippova.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm12e.pdf
• Pulkovo EOP and Reference Systems Analysis Center (PERSAC)

... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Dynamical models of multiple globular cluster populations around massive galaxies . ... Different techniques have been devised to separate multiple GC populations and perform dynamical analyses. ... Within this project, the PhD candidate will examine mock models of multiple GC populations around massive galaxies, devising `blinded' functional tests and comparing the possible sources of bias in different techniques....

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• Data Quality Control and Instrument Modeling
• The Hierarchical Stellar Systems Model Format
• Manipulation of a model

... Dark Matter Ring Modeled around Galaxy Cluster CL0024+17 . ... It is the relatively weak distortions of the many distant faint blue galaxies all over the image, however, that indicates the existence of the dark matter ring. ... A hypothesis for the formation of the huge dark matter ring holds that it is a transient feature formed when galaxy cluster CL0024+17 collided with another cluster of galaxies about one billion years ago, leaving a ring similar to when a rock is thrown in a pond. ...

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• Modelling of light curve of SN87A
• A Kernel Model for Precision Timekeeping
• APOD: 2001 July 10 - Sudbury Indicates Nonstandard Particle Model

... Dark Matter Ring Modeled around Galaxy Cluster CL0024 17 . ... A new observation of gravitationally magnified faint galaxies far in the distance behind a massive cluster of galaxies is shedding new dark on the subject. ... A hypothesis for the formation of the huge dark matter ring holds that it is a transient feature formed when galaxy cluster CL0024+17 collided with another cluster of galaxies about one billion years ago, leaving a ring similar to when a rock is thrown in a pond. ...

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• Астронет > Dark Matter Ring Modeled around Galaxy Cluster CL0024 17
• Sudbury Indicates Nonstandard Particle Model
• Астронет > Sudbury Indicates Nonstandard Particle Model

THE EPIC SIMULATOR AND PILE-UP MODELLING Prashin Jethwa EPIC BOC 2012 7/3/2012 OUTLINE Introduction to the EPIC simulator · What is it? ... Validation Pile-up modelling · Flux losses · Spectral distortions Pile-up mitigation · Correcting spectral distortions The EPIC simulator & Pile Up Modelling | ... Pag. ... 10 PILE-UP MODELLING: flux loss in PN full frame The EPIC simulator & Pile Up Modelling | ... 11 PILE-UP MODELLING: flux loss in PN small window The EPIC simulator & Pile Up Modelling | ...

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• Memory Models
• XMM Radiation Environment Models and Monitor

Bigbang Forum Message . Forums: . ... Discussion Forums | ... The Ekpyrotic [string] Models And The Standard Guth Model. Forum List | ... Post Message | ... Could you outline the differences between the Ekpyrotic [string] models and the standard Guth model? ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• Manual For Telestar By Meade Model #114az - an Astronomy Net Meade Equipment
• New Model: How Do The Sun And Moon Appear To Move Across The Sky - an Astronomy
• Manual Meade Model 114AZ - an Astronomy Net Meade Equipment Forum Message

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