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. ...

Еще в разделе: (Показать все результаты (>25) - rp.iszf.irk.ru/ )

• East Siberian Center for the Earth's Ionosphere Research. Capabilities and

Target Acquisition Reference Information . ... In almost all cases where an onboard acquisition will not work (because the object is in a crowded field, or is variable, or is a moving target), it is sufficient to use an early acquisition to get a WFPC2 or FOC image a few weeks in advance of the GHRS observation. ... Explicit BRIGHT and FAINT limits may be specified if you desire, although there is an increased risk of a failed acquisition unless you are confident of those fluxes. ... MAPs . ...

Еще в разделе: (Показать все результаты (>12174) - www.stsci.edu/ )

• Description of the Reconstruction Methods
• FOCSIM Parameters Fill-out Form
• FOCSIM Parameters fill-out form

... Figure: Massive binary evolutionary track. ... A short glance to this track is sufficient to understand that there are a lot of evolutionary scenario parameters, which affect different stages of the binary evolution. Fortunately, a very limited number of parameters has effect on the compact binary merging rate. ... The most important (and practically unique) parameter changing the galactic binary NS merging rate is the distribution of an additional (kick) velocity imparted to NS at birth. ...

Еще в разделе: (Показать все результаты (>471) - xray.sai.msu.ru/ )

• Initial Distributions of Binary Parameters
• Dependence on the Scenario Parameters and Initial Distributions
• Initial parameters of compact stars

... Number of above the background required for a detection (this parameter is passed to omdetect , see the description of omdetect . ... Half-width of the spectrum extraction region (in pixels, if negative, and in FWHWs otherwise) . ... Offset of the left background extraction region from the edge of the spectrum extraction area; in pixels, if negative, or in FWHWs otherwise. bkgwidthleft . ... Width of the left background extraction region; in pixels, if negative, or in FWHWs otherwise. bkgoffsetright...

Еще в разделе: (Показать все результаты (>15270) - xmm.vilspa.esa.es/ )

... 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. ...

Еще в разделе: (Показать все результаты (>1636) - www.adass.org/ )

• A Python-based IRAF Task Parameter Editor
• VLT Data Quality Control
• Building Software from Heterogeneous Environments

... Mokhovaya st., 11, Moscow, 103907, Russia. ... Proceedings of the 6th IEEE International Specialist Workshop on Nonlinear Dynamics of Electronic Systems, Budapest, Hungary, 16-18 July, 1998 , pp. ... The method for synchronization of drive-response systems on conditions of a large mismatch of parameters is considered on example of the system based on modified Chua's circuit. The approach to information transmission using such method is proposed. ...

Еще в разделе: (Показать все результаты (>509) - www.cplire.ru/ )

• Project 4 - RFBR - Stepantsov, Determination of the space anisotropy of order

Next: Setup Files Up: Frequency Catalog Previous: Frequency Catalog Contents . The parameters of the frequency file tell SCHED over what frequency range the group if usable and on which stations. Most of the parameters are the same as parameters in the setup file since they are meant for direct substitution once the correct frequency group has been identified. ... This will be matched against the station name in the setup file. The name VLBA will be a default for all VLBA stations. ...

Еще в разделе: (Показать все результаты (>23846) - www.atnf.csiro.au/ )

• mslist (Measurement summary and data inspection utility) CentralProcessor 0.11
• Input Parameters to the Self-Calibration Tasks
• casacore: Fitting_module

Next: Equations of condition Up: Extinction and transformation Previous: Extinction and transformation . Bias can also be introduced by improper fitting procedures. For example, the reduction program known as SNOPY, used for many years at La Silla and also at La Palma, uses a simple iterative technique in which some subsets of the parameters are solved for, while others are held fixed; then the ones last solved for are held fixed, while the ones previously fixed are redetermined. ...

Еще в разделе: (Показать все результаты (>2005) - www.sao.ru/ )

• Documentation: LEDA: parameter: bri25
• Geneva parameters
• Documentation: LEDA: parameter: vrot

... IRAF supports two kinds of parameters, auto parameters and hidden parameters, which are treated differently. auto parameters are updated every time a task is run. ... Parameters for each task are contained in `parameter files' in the uparm sub-directory in `myiraf'. ... im > imhead.longheader=yes # explicitly setting <task.param>=<value> im > eparam imhead # Edit the parameter file to update one or more # parameters at the same time # see next section . ...

Еще в разделе: (Показать все результаты (>2307) - hea-www.harvard.edu/ )

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

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. ...

Еще в разделе: (Показать все результаты (>91) - space.univ.kiev.ua/ )

• Additional Parts of Theoretical Astrophysics
• Sun orbital parameters for Computer Ephemeris for 2014 (DE200/LE200).
• Sun orbital parameters for Computer Ephemeris for 2015 (DE200/LE200).

National Research Institute for Physical-Technical and Radio Engineering Measurements IMPROVEMENT OF THE SOFTWARE BERNESE FOR CALCULATION OF THE EARTH ROTATION PARAMETERS ACCORDING TO THE DATA OF SATELLITE LASER RANGING (LAGEOS 1, LAGEOS 2) IN THE MAIN METROLOGICAL CENTRE OF THE STATE TIME AND FREQUENCY SERVICE Tsyba E. N., Kaufman M. B. 141570, Mendeleevo, Moscow region, Russia tel. +7-903-194-7575; tsyba_e_n@mail.ru ABSTRACT Preparatory ...

Еще в разделе: (Показать все результаты (>272) - www.gao.spb.ru/ )

• http://www.gao.spb.ru/english/as/j2014/presentations/suvorkin.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/huang.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm12i.pdf

Following designations of elements/ parameters are used in AMPLE. ... mean anomaly . ... Node . ... Apart conventional orbital elements AMPLE gives possibility to calculate for each minor planet the following often used functions: . ... MOID . ... To calculate MOID user should order the name or the number of the major or minor planet through dialog. ... To calculate CT user should order the name or the number of the major or minor planet through dialog as it is proposed for MOID calculation. ...