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(ASC-FITS-REGION-1.0) FITS region document: see ASC-FITS-REGION-1.0 . 1998 Feb 09: SDS-11.0: FITS function document (superseded by ASC-FITS-FUNCTION-1.2) . ...

Еще в разделе: (Показать все результаты (>4925) - hea-www.harvard.edu/ )

• Jonathan's ASC documents
• The AstroStat Slog model
• Model Spectra for Spectral-Fitting Program

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" . ...

Еще в разделе: (Показать все результаты (>1448) - www.astronomy.net/ )

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

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. ...

Еще в разделе: (Показать все результаты (>41) - rp.iszf.irk.ru/ )

• East Siberian Center for the Earth's Ionosphere Research. Back-scattering
• East Siberian Center for the Earth's Ionosphere Research. Mathematical
• East Siberian Center for the Earth's Ionosphere Research. Maximum usable

... Three SCANs were obtained, two were in the -x direction at a wavelengths of 1400 and 2700 and one was in the +y direction at 2700 . ... Models were created to match the GHRS 1400 (FOC F140M filter) and the 2700 (FOC F278M filter) observations, see Figure 38.1 in which model profiles are offset by one pixel. ... The 1400 scan starts to diverge from the FOC model at ~1.0 arcsec, while the 2700 scan tracks the FOC model scan out to a distance of ~1.4 arcsec before diverging from the model scan. ...

Еще в разделе: (Показать все результаты (>17289) - www.stsci.edu/ )

• Table of Contents
• Modelling
• The Leitherer & Heckman 1995 models

... Both selfcal and gpscal can be given multiple input model images. ... The self-calibration tasks assume that the gains are not dependent on these different aspects of the data ( e.g. the gains are independent of frequency and pointing centre). ... The self-calibration tasks will generally determine the appropriate correspondence between data and model ( e.g. it will associate the data from a particular pointing with a model with the same pointing). ...

Еще в разделе: (Показать все результаты (>24380) - www.atnf.csiro.au/ )

• Probing ISM Models with H observations
• cmodel (Model Image Generator) CentralProcessor 0.11 documentation
• Generating Visibilities from a Model Image

. Hard-copy notes from this video. Back Main Data Handling Page .

Еще в разделе: (Показать все результаты (>679) - www.mso.anu.edu.au/ )

• Lesson 1: Using Uncertainties
• Towards a Truly Unified Model of AGN
• Data Handling Video Tutorials

. Main . Staff . Research . Publications . Conferences . Links . q = M 2 : M 1 = 0.03, e = 0.5, "warm" disk ( с = 0.05), accretion rate = 10 -9 /year. The rotation angle of the apsidal line relative to the observer and through "_" the orbit inclination to the line of sight are indicated in the lower left corner of each diagram.

Еще в разделе: (Показать все результаты (>333) - www.gao.spb.ru/ )

• Model 01_w_03, all curves
• Model 03_w_01, all curves
• Model 05_w_01, all curves

. Reconnecting Science and Art . Album . News . Resources . Web . Links . Who are we? . Previous . Next . List . б? 2010 OASES . [Back To Top] .

Еще в разделе: (Показать все результаты (>3613) - star.arm.ac.uk/ )

• C.J. Butler, Research Astronomer
• A Blinker Model
• EVOLUTION MODELS

. Language [RU/EN] Search: . Home . UP . Research . Projects . Services . Info . News . Events . Personal . Archive . Ionosphere . Ionosounding: . PARUS . Digisonde . Data: . Moscow . St.Petersburg, Kaliningrad . Models: . SM-MIT . --------------------------- . Forecast . Ionospheric weather . Structure . Contacts . N.V. Pushkov . 10/04/2016 01:10 MSK . webmaster@izmiran.ru . Click on the image above to open SMF2 model page . (C) 2007, IZMIRAN

Еще в разделе: (Показать все результаты (>697) - www.izmiran.rssi.ru/ )

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

... The first EGRET catalog ([ Fichtel et al. 1994b ]) used the galactic diffuse gamma radiation model of Bertsch et al. (1993b). ... For the results presented by Bertsch et al. (1993b), the HI and W radio data were deconvolved by integrating the radio data over a velocity interval determined by the endpoints of each distance interval ( ). ... The Galactic radius limit used in the model has been increased to 30 kpc. ... The CR electron spectrum of Fichtel et al. (1991) was used by Bertsch et al. ...

Еще в разделе: (Показать все результаты (>2909) - www.sao.ru/ )

• Extinction and transformation models
• Resource IDs beginning with ivo://svo.cab/models/
• Direct electron imaging-model

The Earth's magnetosphere global structure is conditioned by the interaction of the Solar wind and Earth's magnetic field. ... Solar wind (SW) - the region outside BS; . ... Auroral field lines (AUR) region - the funnel-shape cavity restricted by the geocentric distance of the order of 6 RE, between surfaces formed by magnetic field lines emerged from the polar and equatorial OVAL borders; . ... Fairfield D.H., Average and unusual location of the Earth's magnetopause and bow shock, J. Geophys. ...

Еще в разделе: (Показать все результаты (>1481) - www.cosmos.ru/ )

• Folding Paper Model of Magnetosphere
• Corrected Geomagnetic Coordinates
• (Q-6) Expansion of the Bohr Model

... These Proceedings were prepared in nearly the same manner as the ADASS IV volume (ASP Conference Series, Volume 77), as a single LaTeX document using a style based on the ASP conference style. ... The ADASS V volume (ASP Conference Series, Volume 101), edited by George Jacoby and Jeannette Barnes, contained links to the NASA Astrophysics Data System for as many of the references as possible-we have tried to do the same. ... Previous: Fitting and Modeling in the ASC Data Analysis Environment . ...

Еще в разделе: (Показать все результаты (>1685) - www.adass.org/ )

• Modeling
• Spatial Structure of NGC 6822: An Example for Statistical Modeling of
• Modelling Spectro-photometric Characteristics of Eclipsing Binaries

... 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. ...

Еще в разделе: (Показать все результаты (>915) - www.iki.rssi.ru/ )

• Folding Paper Model of Magnetosphere
• Substorm models [Oulu]
• 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 ...

Еще в разделе: (Показать все результаты (>2789) - www.mrao.cam.ac.uk/ )

• 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

... 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. ...

Еще в разделе: (Показать все результаты (>6089) - www.naic.edu/ )

• Modeling the Spectrum
• sefdPolB_dec07
• pointing

... 87a100np-abp.gif and 87a100np-abp.ps - ut87a100np (solid) and ut87a100abp (dashed, opacity as absorption), scat=true, A . 87a100np-npa.gif and 87a100np-npa.ps - ut87a100np (solid) and ut87a100npa (dashed, scat=false) A . ... e87anp-npa-abp.gif and e87anp-npa-abp.ps - early light curves for ut87a100np,ut87a100npa and ut87a100abp, data from Shelton and Lapasset, 1993 . ... 100np-curves.gif and 100np-curves.ps - light curves for ut87a100np (scat=true) and ut87a100npa (scat=false) . ...

Еще в разделе: (Показать все результаты (>1796) - www.sai.msu.su/ )

• APOD: 2007 May 16 - Dark Matter Ring Modeled around Galaxy Cluster CL0024 17
• APOD: 2015 April 21 - Vesta Trek: A Digital Model of Asteroid Vesta
• A Kernel Model for Precision Timekeeping

. Scientific Organizing Committee . Scientific Rational . SOC . Programme . Luis Aguilar . Mexico . Amina Helmi . Netherlands . James Binney ( chair ) . UK . Jacques Lepine . Brazil . Herwig Dejonghe . Belgium . Alice Quillen . USA . Ken Freeman . Australia . Annie Robin . France . Ortwin Gerhard . Germany . Natalia Sotnikova . Russia . Naoteru Gouda . Japan . Contacts: . E-mail: binney@thphys.ox.ac.uk . Print: PDF . Back to Top

Еще в разделе: (Показать все результаты (>339) - www.astro.spbu.ru/ )

• Model of clusters
• Modelling the Milky Way in the Era of Gaia - JD5 Rationale
• Modelling the Milky Way in the Era of Gaia - JD5 programme

... Elena Seifina and Lev Titarchuk "On the nature of the compact object in SS433: observational evidence of X-ray photon index saturation" 2010, Astrophysical. ... A.M. Cherepashchuk, R.A. Sunyaev, E.V. Seifina, E.A. Antokhina, D.I. Kosenko, S.V. Molkov, N.I. Shakura, K.A. Postnov, A.N. Timokhin, I.E. Panchenko "INTEGRAL Observations of SS433: Analysis of Precessional and Orbital X-ray Periodicities" 2007, 6th INTEGRAL Workshop, Eds. S. Grebenev, R.A. Sunyaev, p.411 (astro-ph/0610235) . ...

Еще в разделе: (Показать все результаты (>21) - uranus.sai.msu.ru/ )

• Elena Seifina

... 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....

Еще в разделе: (Показать все результаты (>66244) - www.eso.org/ )

• Manipulation of a model
• Astroclimatology, Forecast Models
• Data Quality Control and Instrument Modeling

... We find a transition of LBV star from the LBV instability strip to the region of classical WN for the first time. ... Numerical modeling of the atmospheres of these objects are very important for understanding the evolutionary relationship WR and LBV stars, as well as of the physical causes of LBVs variability. We studied spectra of two very luminous stars in the M33 galaxy - LBV V532 and late WN star FSZ35. ... Bottom: The spectrum of FSZ35 with the final model . ...

Еще в разделе: (Показать все результаты (>338) - mavr.sao.ru/ )

• SAO RAS home page
• The dust jets in the nucleus of comet 29P/Schwassmann-Wachmann 1
• Solar system sector, archive 1993