This is how a typical dispersion modeling result looks when shown as a map. ... Their numerical values are shown at the top. White normally means no data, but high values may be also shown as white if above the fixed high limit (that is, if no automatic normalization is used for colors). Note that calculations were done both for cell positions and for station positions, so both are colored. PO territories are filled by color corresponding to the average value of cells overlaying them. ...

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• PC index
• Geomagnetic Kp Index
• ФОРМАТ ЗАПИСИ В БАЗЕ ДАННЫХ НА CD-ROM

This document explains values, tables and other matters on solar physics computing pages. ... is040423.ete : SAHA-S tables, interpolation values: T, rho, X. Z is fixed at 0.02. See reference above. opal2005.etf : OPAL EOS, interpolation values: T, rho, X, Z. Downloaded from OPAL site , marked there as "2005", seems to be unpublished. opal2001.etf : OPAL EOS, interpolation values: T, rho, X, Z. Rogers F.J., Nayfonov A. Astrophys. ... The following values can be calculated: . ... dimensionless . ...

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• Equation of state for solar modeling
• Solar modeling input physics (thermodynamics, opacity, nuclear reactions)
• Descriptor index

Next: *period* - Period search Up: *fft* - Period search Previous: A summed or incoherent . The distribution of coefficient values for a single FFT is exponential if the original data contain no periodic signal. ... Significant coefficients will appear beyond the high-value end of the normal distributions. ... xt> fft.histogram_bi=0.5 # if necessary, adjust number for an aesthetic plot xt> ftpplot input table file: rp90_ftp The plot will appear on the screen. ...

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• Mapping Pixel Values to Screen Intensity
• Model Spectra for Spectral-Fitting Program
• The AstroStat Slog Blog Archive P Values: What They Are and How to Use Them

Next: DOMKA Up: Details of SCHED Parameters Previous: DEBUG Contents . Normally, SCHED eliminates stations for which the source is not up if they are using a disk recording system. DODOWN with no argument overrides that behavior and keeps stations in scans regardless. ... Without DODOWN , SCHED will also take a station out of a scan if the predicted slew time is such that the antenna will not reach the source before the scan end. ... Default: Stations taken out of scans ( DODOWN not zero) . ...

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• TPMODE
• Keyin Free-format Input
• NDRIVES

Stellarium 0.12.3 . ... Classes . ... AngleSpinBox Class Reference . A spin box for displaying/entering angular values. More... #include < AngleSpinBox.hpp > . ... virtual voidљ . ... Set the value to default 0 angle. ... AngleSpinBox (QWidget *parent=0, DisplayFormat format= DMSSymbols , PrefixType prefix= Normal ) . ... Set the display format. ... the value to set, in decimal degrees. void AngleSpinBox::setDisplayFormat . ... the value to set, in radians. void AngleSpinBox::valueChanged . ...

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• Stellarium: Member List

... #*********************************************************************** from checklist_init import UNKNOWN, PASS , FAIL import os import spss_tk_util if spss_tk_util.GUI_AVAILABLE: from Tkinter import Checkbutton, IntVar, Label, Button, W, E, NORMAL , DISABLED from Tkinter import TOP, X, RIGHT, LEFT , Toplevel, Frame, YES, Y, BOTH, RAISED from Tkinter import BOTTOM, Scrollbar, ...

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• http://www.stsci.edu/spst/UnixTransition/doc/StickyForm.py
• CSPICE Routines: BODVCD_C
• CSPICE Routines: BODVRD_C

... 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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The power in the 6 Mhz band of each tv Station is monitored using the hilltop monitoring system . There are 5 frequency bands of the rfi monitoring system that contain tv stations: (70, 165, 235, 550, and 725 Mhz). ... This gives 74 measurements per band per day. ... The red line is the median power in the band for the day. ... The station is probably turning on for half a day and the median is alternating between catching the on and off power levels. date . daily median power . ...

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• Approximating calvalues over wide bandwidths
• a2584
• gps rfi aug08

... FIELD | ... public class Menus . ... ImageJ . ... static char . ... static int . ... Returns the size (in points) used for the fonts in ImageJ menus. static java.lang.String . ... Returns a list of the plugins in the plugins menu. static java.lang.String . ... Field Detail public static final char PLUGINS_MENU . ... public static final char IMPORT_MENU . ... public static int installPlugin (java.lang.String plugin, char menuCode, java.lang.String command, java.lang.String shortcut, ImageJ ij) . ...

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Wang-Landau sampling method Wang­Landau method is the random walk in the energy space with a flat histogram. ... If not, accept the new state with probability g(Ek) / g(Ek+1), Otherwise keep the current state unchanged (not-accept). ... MN times, ... f = f1/2, g(E0) = 1 , reset histogram H(E)=0 The algorithm may be stopped with some small value of f.e. f close enough to unity, log f = 10-9 DoS of Ising model Exact - Beale, PRL 76 (1996) 78 DoS g(E) for Ising model 16x16. ...

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• V.G. Petukhov (Khrunichev State Research and Production Space Center).

... SELECT file, title, rank(ts_vec, to_tsquery('create schema')) FROM postgresql_manual WHERE ts_vec @@ to_tsquery('create schema') ORDER BY rank(ts_vec, to_tsquery('create schema')) DESC LIMIT 5; file | title | ... CREATE SCHEMA | ... SELECT file, title, rank('{0, 0, 0.01, 0.99}',ts_vec_tb, to_tsquery('create aggregate')) FROM postgresql_manual WHERE ts_vec_tb @@ to_tsquery('create aggregate') ORDER BY rank('{0, 0, 0.01, 0.99}', ts_vec_tb, to_tsquery('create aggregate')) DESC LIMIT 5; file | ...

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• Sternberg Astronomical Institute
• Zen: sncat design
• Moscow University from SAI

. Pulkovo Observatory of Russian Academy of Sciences is situated . near Saint-Petersburg. It was founded in 1839. 196140, Saint-Petersburg, Pulkovskoye chaussee 65/1 . English version . Russian version . This page has been accessed times since May 1, 1999.

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• PULK GNSS station

... The Earth orientation parameters UT1 and polar motion (x pol ; y pol ) are relat­ ed with the values of UT0 and VOL obtained from the LLR analysis for a station with geocentric longitude and latitude (–; OE) by the following expression: 7 UT0 \Gamma UTC = UT1 \Gamma UTC + (x pol sin – + y pol cos –) tan OE 15 V OL = x pol cos – \Gamma y pol sin – At least four normal points for each station--reflector pair at one day were accepted for the diurnal UT0 estimations. ...

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• http://www.ipa.nw.ru/conference/2002/sovet/PS/GUSEV2.PS
• Keywords_129
• Values of asteroid masses

... This noise can be reduced by replacing the pixels with an average of the surrounding values using a linear filter. ... The effects of applying linear filters to a CCD frame is shown in Figure . Figure: Different digital filters applied on a CCD image: (A) original, (B) block filter, (C) smooth filter, and (D) Laplacian filter. ... To remove stellar images from a picture of comet Halley, the results of applying different non--linear filters to the frame are given in Figure . ...

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• Example rc file
• Setting the Low and High Cuts
• Errors in the Steady State and Quasi-SS Models

This Directory contains mean hourly, mean daily and mean monthly values of cosmic ray intensity recorded by World Network NM stations to the end of 2011. ... CD is created in WDC for STP, Moscow and IZMIRAN. ... This directiry contains catalogue Corrected for pressure and verificated data in WDC for STP, Moscow . This directiry contains catalogue Corrected only for pressure but Original data in WDC for STP, Moscow . ... 20 May - 22 July 1972, M., 1975 6. 27 March - 22 July 1972, M., 1975 7. ...

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• Catalogue 2 of WDC-B
• IRT in 1951
• IRT in 1953

... 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
• SCL Sfit SLV Commands
• FFIT - Command Syntax

... References: %observed energy levels: NIST database (http://physics.nist.gov/cgi-bin/AtData/main_asd) %theoretical energy levels: Aggarwal, K.M., Keenan, F.P., 1998, J.Phys.B, 31, 4545 %comment: Aggarwal Keenan give only LS state energies % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % P.R. Young - 27-May-03 . ...

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• Color Values
• Procedures for Data Reduction
• Re:return values

MAIN CHARACTERISTICS BASIC MODIFICATIONS TEST RESULTS . ... integrated drop tests in order to verify the strength of DM modified shell and equipment attachment points, functional check of new chairs and DM structure, determination of shock impacts onto the crew to verify landing safety; . ... nominal landing with the main parachute system (MPS) - drop #1 took place on December 24, 1998; . ... reduction of shock g-loads values at landing in accordance with decrease of landing speeds. MAIN | ...

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• S.P. Korolev RSC Energia - International Space Station

polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

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polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

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• Bias correction of visibilities
• ESO - How do I interpret the SEQ TIME keyword values?
• ESO - Negative pixel values in the 2D spectrum image are not being ignored by