Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Investigations of the ionospheric response to strong magnetics storms which are usual for our latitudes, are of great interest. ... In the figure, we present ionospheric parameter dynamics during three perturbed days in July 2000. ...

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• East Siberian Center for the Earth's Ionosphere Research. Modelling, secondary
• East Siberian Center for the Earth's Ionosphere Research. Capabilities and
• East Siberian Center for the Earth's Ionosphere Research. Specific character

... Posts tagged ?nuisance parameter? ... Ah ha~ Once I questioned, ?what is systematic error?? (see [Q] systematic error. Thanks to L. Lyons? work discussed in [ArXiv] Particle Physics , I found this paper, titled Systematic Errors describing the concept and statistical inference related to systematic errors in the field of particle physics. ... Continue reading ?systematic errors? ... Comment . ... ArXiv]4th week, Mar. ... Entries RSS . Comments RSS . ... Entries (RSS) and Comments (RSS) . ...

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• Parameters
• Editing Files and Parameters
• Model Spectra for Spectral-Fitting Program

. ___________________________________________________________________ The Electronic Universe Project e-mail: nuts@moo.uoregon.edu

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... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...

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• Parameters of the 41 Dra system components
• проект SCORPIO-2: parameters
• SCORPIO parameters

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Quasi-stationary electron distributions for the different values of the particle escape time. ... The electron-cyclotron maser instability is widespread in the Universe, producing, e.g., radio emission of the magnetized planets and cool substellar objects. ... The model used takes into account the radiation escape from the source region and the particle flow through this region. ...

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• Sfit Control Language: Classified Listing
• lte-codes: sterne model atmospheres
• SCL Sfit SYN Commands

Next: File Formats Required Up: OPTOPUS Commands and Previous: Optopus commands . Below follows a description of all parameters that can be set by the SET/OPTOPUS command, the commands which use these parameters and the default values. ... If an OPTOPUS command the default value is not used the command will, in addition to actual OPTOPUS operation, also overwrite the setting of this parameter and hence will change the default value. ... set the equinox . ... Table: Command parameters . ...

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• Line parameter measurements
• Mean astrophysical parameters from LEDA
• Summary of the parameters handled by the user:

... Meta Index / Home Page This section documents the parameters recognized by this task (if any). Parameter . Mand . ... Default . Constraints . ... real list . ... order . ... integer . reflection order . instrument . ... RGS1 . RGS1, RGS2 . ... real . ...

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Next: Other parameters of the Up: The Model Previous: Initial binary parameters . As we only deal with initially massive binary systems (their primary's mass is higher than 10 ), which are capable of evolving off the main sequence during less than years, the compact stars left behind stellar evolution are (in the case of the most massive stars) NSs and BHs. ... For a NS belonging to a binary, the evolution complicates as the secondary star evolves: for example, (recycling), etc. ...

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• Other parameters of the evolutionary scenario
• The Effect of Relativistic Wind on Accretion Flow Parameters
• The Gravimagnetic Parameter

Orbital data : INTERBALL AZ GSE and GSM cartesian coordinates, GSE cartesian velocity (once per 10 minutes). ... Magnetic field data from IMAP experiment. Magnetic fileld absolute value and magnetic field index (the difference between absolute value and model value), status flag. ... Counts of H+ and O+ ions are accumulated during one spin period by detectors D6 (antisunward looking), D8 (spin plane), D10 (sunward looking) of TRICS2 subsystem (1.0-30 keV). ... TRICS1, TRICS2, TRICS3 subsystems: . ...

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• INTERBALL-TAIL KP rules
• ENERGETIC PARTICLE EXPERIMENT DOK-2
• INTERBALL-AURORAL KP plots

This page will contain brief descriptions (incl. refs) and parameter lists for most popular models of small scattering particles used in applications. single particle: . homogeneous particles: . sphere - m, r . infinite cylinder - m, r, alpha . finite cylinder - m, r, l, alpha . spheroid - m, a, b, alpha . ... Chebyshev particle - m, r, n, eps, alpha . ... irregular surface ... bi-sphere - m, r, ... multi-sphere - ... fractal aggregate - ... inhomogeneous particles: . ...

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• Linear polarization: wavelength dependence
• AI SPbU library of scattering codes
• Rayleigh and Rayleigh-Gans-Stevenson approximations

Subject, Problems and Objects of Theoretical Astrophysics. ... Stellar Photospheres, Their Features. ... Physics of Continuous Radiation Absorption in Stellar Photospheres. ... Continuous Radiation Absorption in Stellar Photospheres of Various Spectral Classes. Solar Type Photospheres. ... Characterisics of Absorption Lines. ... Interstellar Absorption Lines, Their Features. ... Physical and Dynamic Features of Interstellar Medium, Which Follows from Observations of Interstellar Absorption Lines. ...

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• MISSION WARNING
• Sun orbital parameters for Computer Ephemeris for 2014 (DE200/LE200).
• Sun orbital parameters for Computer Ephemeris for 2015 (DE200/LE200).

The current set of keyword-value pairs of a task can be monitored by typing ESC K while the name of the task is present in the User Command Area. This causes (part of) the Common Output Area to be overlaid with a display containing the current user input parameters of the task. ... If there is currently a set of parameters displayed on the screen (as the result of typing ESC K ), these parameters will be edited; otherwise the name of the task is derived from the User Command Area contents. ...

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• User Parameters - Continuum imaging CentralProcessor 0.11 documentation
• List of Frequency File Parameters
• SCINTILLATION PARAMETERS FOR 49 PULSARS

... number of particles integer, parameter :: max_list = 100 ! max number of particles per cell integer, parameter :: ncell = 20 ! ... cell size real(dp) posn(3, npart) ! ... initialise cell list call init_cell_list(npart, ncell, max_list, cell_size, posn, & cell_num, cell_list) ! now go and do something interesting with it... contains subroutine init_cell_list(npart, ncell, max_list, cell_size, posn, & cell_num, cell_list) implicit none integer, parameter :: dp = kind(1.0d0) integer npart ! ...

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• Abstract
• PPEUC Programme - Cosmic Microwave Background Workshop
• B Bayesian value for

EXPERIMENT . ... Charged energetic particles (Ee=40-200 keV; Ei=0.05-150 keV) composition and anisotropy. ... IKI, Moscow, Russia . ... University of Thrace, Xanthi, Greece . ... Energy spectra, angular distributions and time variations of electrons (E=15-400 keV) and ions (E=20-1000 keV). ... IMBP, Moscow, Russia . ... Moscow University, Moscow, Russia . ... IPG, Moscow, Russia . ...

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• MPS,SPS,VDP: measurements of charged particles
• DOK-2 Results Page
• Multipoint correlations of the solar wind parameters observed by several

Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents . The parameter file contains information for CONSTRICTOR on the location of the raw data files, start and stop times, integration time, etc. ... The parameter file, YYYY-MM-DD.par , can now be created using the rawlist procedure of . ... Check beginning and tail of the listing for each file. ... Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents Christian Hummel 2015-04-28 ...

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• CONSTRICTOR parameters for astrometric reductions
• Parameters
• Stellar parameters from calibrations of spectral types

... Program of the Course of Radio Astronomy . Moscow State University , Physics Department , Astronomy Division , 4 th year, 60 hours in total) . ... Molecular maser emission. ... The emission of the interstellar neutral hydrogen. ... Pacholczyk, A. G. Radio Astrophysics, W. H. Freeman & Co., ... Frontiers of Astrophysics, Avrett, E. H., ed., Harvard University Press, Cambridge, Mass., ... Kaplan, S. A., Pikelner, S. B. The Interstellar Medium, Harvard University Press, Cambridge, Mass., ...

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• Passing arguments to the shell

... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...

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• TwoFitlines: An Spectrum and Line Analysis Tool
• Recent Advances in Parameter Estimation in Astronomy with Poisson-Distributed
• Enhanced HST Pointing and Calibration Accuracy: Generating HST Jitter Files at

Welcome to Starburst99 . ... Starburst99 Services | ... Starburst99-Mappings . ... Run Your Own Starburst99 Simulation . ... Fixed Mass . Total Stellar Mass x10 6 M . ... Mass Boundaries for IMF . ... 0.0004 0.004 0.008 0.020 0.050 . Padova AGB 0.0004 0.004 0.008 0.020 0.050 . ... 0.001 0.004 0.008 0.020 0.040 . Geneva High 0.001 0.004 0.008 0.020 0.040 . Geneva v00 0.001 0.002 0.008 0.014 0.040 . Geneva v40 0.001 0.002 0.008 0.014 0.040 . ... 0.001 0.008 0.020 0.040 . ...

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• Optional Parameters [Optional_Parameters]
• MultiDrizzle parameter tables
• CCD Parameters table

... Публикации и издания Публикации профессорско-преподавательского состава СГАУ Издания проф. Сосниной Т.Н. Biosphere: Analysis of Value Parameters . ... Besides, the ways of saving the use value and value properties of biosphere are analyzed. The expediency of transformation of two-criterion theory of value into the three- criterion theory of the balance of value, where the ecologic component performs the function of the key criterion has been founded. ... BIOSPHERE USE VALUE OF THE PRODUCT: MAIN . ...

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Next: Program use Up: Description of program searchdup Previous: Description of program searchdup . Parameter input is done with a graphic user interface. ... Input file: Name of the input catalog file. It has to be formatted, one record per source/observation, according to the format used in the Arcetri observations and source archives. ... Minimum number of observations per source Source with less than this number of independent observations are not included in the output file . ...

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• Where are the tunable parameters of the kernel?
• Kernel tunable parameters
• Tunable Kernel Parameters?