In order to calculate the line profile of a given absorption line for atomic species Z with a wavelength LAMBDA (in Angstroms) and a microturbulent velocity VT (in km/s). ... mode . ... 1) The input model may contain more than one model (i.e. it may be an entire grid of models). Spectrum will cycle through this grid NMOD times, omitting NSKIP-1 models from the . ... However, the input data following MODE must be repeated NMOD times in order to obtain equivalent results for each model in the grid. ...

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• sfit help file
• FFIT - Command Syntax
• Spectrum - control

... This section describes how to copy a file between two VMS systems using the COPY command, and between a VMS system and another computer using FTP or Kermit. Remote file access may be made on either the file or record level, but only file level access is discussed here. To access a file, you use normal VMS commands, such as COPY or TYPE , but you specify the file name differently. ... It is also possible to automate your file transfers using scripts in conjunction with the Kermit TAKE command. ...

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• CSPICE Routines: PL2NVC_C
• CSPICE Routines: LSPCN_C
• CSPICE Routines: PL2NVP_C

... The models provided are: . abs - absorption of x-rays by neutral gas with solar abundances. parameter 1 = . ... parameter 2 = . ... normalization - logarithmic value of the flux density at 1 keV in units of keV cm -2 s -1 keV -1 . ... normalization - logarithmic value of the normalization of the gaussian in units of keV cm -2 s -1 . ... absorption ( params )* model ( params ) . ... A single value for the normalization (i.e., fixed normalization) will force the program to use that value. ...

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• *xflux, hxflux* - Calculation of X-ray Flux
• The AstroStat Slog normalization
• The AstroStat Slog Blog Archive my first AAS. VI. Normalization

... the shutters, loads . ... We have shutter/receiver protection to protect the receivers when we transmit with one of our transmitters (sband,430, hf). ... this is also controlled by the 430 ch load/antenna switch. closed always wins . ... shutter - open,close, or query the receiver/radar shutters . ... When the 430 dome is being used, we want to close all shutters, but leave the 430 dome receiver under control of the ch load/antenna switch (above the oscilloscopes in receiver room). ... shutter close...

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• software_downloads
• CIMA Auto-Observing
• spectrometer counts to kelvins

Next: Creation of the Up: Typical Run Previous: Initialisation of the . The command CREATE/PSF creates a 1D image of a normalized gaussian centered in 0. Command: . NAMEP : output image . FWMM : full width at half maximum of the instrumental response (?) ... This image is to be used by the command COMPUTE/ABS ; any other (non gaussian) PSF can be used provided it is centered in 0, normalised and has the same step size as the synthetic image. ... Mon Jan 22 15:08:15 MET 1996 ...

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• Normalization and Fitting
• Cleaning Images
• cloud

... You are here: start €Ё correlator €Ё mpiscript . ... MPI . ... An important one in most cases is MPI_Comm_rank() which returns an ordinal integer number to each instance . ... Type $ mpirun -np 3 -machinefile machines env . ... On cuppa it is OMPI_MCA_ns_nds_vpid $ mpirun -np 6 -machinefile machines env | ... usr/bin/perl use Env; Env::import(); $rank=$OMPI_MCA_ns_nds_vpid; if ($rank == 0) { print "I am zero\n"; } elsif ($rank < 5) { print "I am $rank\n"; } else { die "Nothing to do\n"; } . ...

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• uvamp
• casacore: casa::Normal Class Reference
• imcfn

... Meta Index / Home Page / Description / Specifying source region shapes . When radiusstyle =`contour', the task calculates the source region shape as an elliptical locus which approximates the contour of the PSF at a given flux value. ... Clearly, in order to calculate the shape of such a flux contour, it is necessary firstly to normalize the PSF to the source brightness and secondly to determine the flux level (in `brightness' units per pixel) at which to find the contour. ...

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• Procedure
• Environment variables

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... The algorithm and appropriate program for decametric radiosignal propagation conditions prediction for paths from 500 to 9000 km have been developed at ISTP SB on the basis of normal wave method (AltyntsevaB.I,Iliyin N.V., Kurkin V.I. and others //Decameters channel simulation on the base of normal wave method . ... Solar activity indices are chosen automatically from the prediction date from the database . ...

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... 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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• UnsharpMask (ImageJ API)
• GaussianBlur (ImageJ API)

... We consider stars with a constant (solar) initial chemical composition. Before the Roche lobe overflow, the components evolve as single stars (see for details LPP96). ... If the mass transfer onto a normal star occurs on a time-scale ten time shorter than the thermal Kelvin-Helmholz time for this star or a compact star is engulfed by a giant companion (e.g. as a result of the kick), the common envelope (CE) stage of the binary evolution is set in (Paczynski 1976). ...

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• Stellar Winds From Normal Stars
• Star Formation Rate and Normalization of Stellar Populations
• Principal Evolutionary States of Normal Stars

... 6.1 Specified, computed, and actual values . ... 6.2 Inheritance . ... Once a user agent has parsed a document and constructed a document tree , it must assign, for every element in the tree, a value to every property that applies to the target media type . ... User agents must first assign a specified value to a property based on the following mechanisms (in order of precedence): . ... By default, rules in an author's style sheet override those in a user's style sheet (see cascade rule 3). ...

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• Feature enhancement: normalizing
• Explanations for solar physics computing page
• Long description of how floats overlap with boxes in normal flow

... MIPT Solid State Physics Department . ... Interacting Electrons in Normal Metals . ... The course is an introduction to interacting Fermi-particle physics and intended for future experimentalists. ... Hartree-Fock approximation. ... Linear reaction function. Calculation of density-density reaction function. Relation of density-density reaction function to compressibility of Fermi liquid and thermodynamic state density. ... Density-density reaction function of free Fermi gas in long-wave limit. ...

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Modules | ... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Modules . ... Description: . User authentication using MD5 Digest Authentication. Status: . Extension . ... This module implements HTTP Digest Authentication ( RFC2617 ), and provides a more secure alternative to mod_auth_basic . ... Questions on how to manage the Apache HTTP Server should be directed at either our IRC channel, #httpd, on Freenode, or sent to our mailing lists . ...

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• HwB: SGI Video Connector (Offline)
• Starting Apache - Apache HTTP Server
• HwB: A1000 to Amiga Parallel Adapter (Offline)

The NTP standard specifies an extension which provides cryptographic authentication of received NTP packets. ... The specification allows any one of possibly 4 billion keys, numbered with 32-bit key identifiers, to be used to authenticate an association. ... In the case of MD5, the keys are 64 bits (8 bytes). xntpd reads its keys from a file specified using the -k command line option or the keys statement in the configuration file. ... A zero key in NTP format would be specified as 8080808080808080 . ...

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• Zen: sncat design
• Reference Clock Options
• APOD: 2005 August 8 - Mars to Appear Normal this August

OptInt PmWiki : Pm Wiki / Wiki Style Examples . Wiki styles | ... PmWiki uses WikiStyles for styling text with color and other attributes. PmWiki 2.0 introduced the ability to control the styling further and to even place styles on blocks. ... In addition, an author can define a style "shortcut" by using the define= property. For example, to define a style of %red% , one can use: . define=mystyle color=red% Here is some %mystyle% red text created using a style shortcut. ...

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• OptInt PmWiki : PmWiki / Basic Variables
• Bojan Nikolic -- Calculating dispersive path delay due to the atmosphere
• Computing dispersive atmospheric delay with AATM

... We cannot use for this purpose equivalent widths and profiles of HI lines (well known criteria of atmospheric conditions for normal supergiants), since these lines are strongly distorted in the spectrum of IRAS04296 as seen in Fig. ... Figure: Upper: iron abundance FeI (circles) and FeII (crosses) calculated for IRAS04296+3429 with model parameters , and using lines with different excitation potentials EP of a low level; bottom: the same as a function of the equivalent width W . ...

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• Linux I/O port programming mini-HOWTO: Using I/O ports in C programs
• di_eks
• From Power Up To Bash Prompt: Lilo

Computer Ephemeris. Reduction quantities for Sidereal time. Explanations. Each row contains for the date specified at 0 h of Time Dynamical Sidereal: . sidereal julian day, . interval from date to mean epoch T m expressed in julian years, . reduction quantities A+A', B+B', C, D, (all in seconds of arc), E (in 0.0001s), A', B' (in 0.001). The same table, but for moments, expressed in Dynamical Time is to be found on 'Reduction. Dynamical time.' page. ...

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• Reduction quantities for Dynamical time. Explanations for Computer Ephemeris.
• Ephemeris of Saturnian rings. Explanations for Computer Ephemeris (DE200...
• Explanations to ephemeris for physical observation of the planets for Computer

... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...

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• Database of Optical Constants -- Misc: computer codes

... Restrictions ) are used. If specified form of output is EMP then astrometric equatorial coordinates are printed in the form usual for Ephemerides of Minor Planets, with formal precision of 0.01 minute of time in R.A. and 0.1 minute of arc in declination. ... It should be noted that the near-opposition ephemerides are not calculated for bodies/ points with numbers from –12 to 0 (in case they are included into task for computation of such ephemerides only their names are displayed in the results). ...

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• Keywords_129
• ENGAMPLE

... Linear limb darkening coefficients are taken from tables published by Van Hamme (1993, AJ 106, 2096). limb_stars Compute limb darkening fit coefficients for all stars. limb_star ( spectrum _char , filter _char ) Function. Return linear limb darkening coefficient integrated over specified bandpass. Example: print, limb_star('G0I','V') . ... Return factor to multiply the uniform disk diameter with in order to get a limb darkened diameter using the specified linear limb darkening coefficient. ...

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• Model manipulation
• Astrometry
• PWVmonitor.html