To change the Scaling Function (how pixel values are binned into color levels): . ... For example, the basic grey-scale color map specifies no intensity for any color at the lowest color level, full intensity for all colors at the highest color level, with the red, green and blue intensities varying linearly for intermediate levels. ... At low bias, low color levels (i.e., low pixel values) will have non-zero intensities, while at high bias only high pixel values will have non-zero intensity. ...

... User Guide ] Task: uvdump Purpose: Generate an output text file of information from a visibility dataset. ... For each data record selected, an line is produced in the output text file. Each line can consist of several values. Key: vis The input UV dataset name. No default. ... Note these names cannot be abbreviated. real Real part of a correlation. imag Imaginary part of a correlation. amp Amplitude of a correlation. phase Phase of a correlation, in degrees. flag Data flag. ...

... FIELD | ... public interface Blitter . ImageJ bit blitting classes must implement this interface. ... static int . ... dst=dst+src . ... Field Detail static final int COPY . ... Constant Field Values . static final int COPY_INVERTED . ... static final int COPY_TRANSPARENT . ... static final int ADD . ... static final int SUBTRACT . ... static final int MULTIPLY . ... static final int DIVIDE . ... static final int AVERAGE . ... static final int DIFFERENCE . ... static final int AND . ...

Table of Contents | ... The string literals in this appendix can be used to specify colors in the JavaScript alinkColor, bgColor, fgColor, linkColor, and vLinkColor properties and the fontcolor method. You can also use these string literals to set the colors in HTML tags, for example < BODY BGCOLOR="bisque"> or < FONT COLOR="blue">color me blue</FONT> Instead of using the string to specify a color, you can use the red, green, and blue hexadecimal values shown in the following table. Color . ...

. To display the current value of all options enter the command: :set all . To display the value of those options whose values have been reset from their default enter the command: :set .

- mssql $Id: attach_mssql_basic.sql,v 1.9 2003/08/30 15:47:39 acydburn Exp $ */ BEGIN TRANSACTION; /* -- attachments_config */ INSERT INTO phpbb_attachments_config ( config_name , config_value ) VALUES ('upload_dir','files'); INSERT INTO phpbb_attachments_config ( config_name , config_value ) VALUES ('upload_img','images/icon_clip.gif'); INSERT INTO phpbb_attachments_config ( config_name , config_value ) ...

This module provides for server-side imagemap processing. ... Configurable generation of imagemap menus. The lines in the imagemap files can have one of several formats: directive value [x,y ...] . ... The directives can come in any order, but are processed in the order they are found in the imagemap file. base Directive . ... Module: mod_imap . ... Its value is overridden by a default directive within the imagemap file. ... Its value is overridden by a base directive within the imagemap file. ...

... STScI has undertaken a project to place all HST keyword information in one source, the keyword database, and to provide a mechanism for making this keyword information accessible to all HST users, the keyword dictionary, which is a WWW interface to the keyword database. ... Along with forming the headers for the science data, most keyword values are ingested into HST archive catalog fields where they are accessible for archive searches and data characterization. ...

... fork() . ... A process is basically a single running program. ... System is prototyped in <stdlib.h> . ... Each command and sorresponding arguments are put in a args array */ /* execvp is called to execute these commands in child process */ /* spawned by fork () */ /* cc -o fork fork .c */ #include stdio.h #include sys/types.h #include unistd.h main() { char buf [1024]; char * args [64]; for (;;) { /* * Prompt for and read a command. */ printf( Command: ); if (gets( ...

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 . ...

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 . ...

Input function: . Input X: .

This widget allows you to offset the telescope. ... Offset type : one of "Object Arc", "Object Arc XY" or "Boresight". ... This is motion on the sky or instrument, so don't worry about cos(dec). ... If you want to move that point (e.g. center your object along a different bit of the slit), then use a boresight offset. ... Note that a +X object xy offset will move the sky in the -X direction on the focal plane, because you are centering something in the +X direction on the boresight. ...

... Астронет | ... планета Астронет | ... Астрономия в России | ... История астрономии . ... Любительская астрономия . ... Кривая блеска GRB 030329 . ... Includes most data through GCN 2276 . Light curve of posted GCN observations of GRB030329, including AAVSO observations, by Melissa Nysewander (UNC-Chapel Hill) . ... Публикации с ключевыми словами: гамма-всплески - оптические ореолы гамма-всплесков . ... Самый далекий, самый желанный . GRB 090423: самый далекий взрыв . ...

The kinematical properties of the fragment ejection processes in the events that produced the presently known asteroid families have long been poorly known due to the presence of a couple of unknown angles (the true anomaly and the argument of the perihelion of the parent body at the epoch of the family formation) in Gauss' equations. ... In these cases, we show that the unknown angles can be reliably determined, and the ejection velocities of the fragments can be fairly well reconstructed. ...

Microsymposium 38, MS082, 2003 (A4 format) EVALUATING THE STRUCTURE OF THE SURFACE LAYER OF MERCURY. ... Photometric Analysis of the Lunar Surface Analogue. ... The phase function obtained directly on some segments of the lunar surface: 1- phase function of the Moon, 2 - phase function of Mercury, 3 - phase function of segments, converted to the lunar phase function system (correlation 0.8), 4 - phase function of segments, converted to the Mercurian phase function (correlation 0.9). ...

RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . Research results on fast active processes General information Main characteristics of the Radio telescope Observing programs General view of the antenna array Main research areas Principle of generation of radio images Radio telescope's beam Receiving systems Main characteristics of the base receiving-recording complex Calibrations Data archive and databases ... Distribution of the recorded spikes in duration . ...

Multi-Frequency Synthesis in K-band . The Multi-Frequency Synthesis (MFS) permits to realize a good quality imaging of the continuum radio sources in short time. ... The RadioAstron mission will operate one K-band circular polarized channel at fixed frequency 22,232 GHz. ... In general one K-band RadioAstron channel with fixed frequency will be unchanging and compatible with all the ground radio telescopes. ... Progress of the RadioAstron Project in Pictures . ...

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Magnetic Stars, 2011, pp. 153 ­ 156 Ab out the Dep endence of the Rotation Velo city of CP Stars on the Magnetic Field Glagolevskij Yu. ... Based on the observational data of the average magnitudes of the surface magnetic field strength Bs for a number of chemically peculiar stars we investigate the dependence of the rotation period on the magnetic field. ... Now the periods of rotation P and the average values of the surface magnetic field Bs are known for more than 50 magnetic stars. ...