... Directives | ... Apache HTTP Server Version 2.2 . ... The most important directives used to control this MPM are ThreadsPerChild , which controls the number of threads deployed by each child process and MaxClients , which controls the maximum total number of threads that may be launched. ... Two directives set hard limits on the number of active child processes and the number of server threads in a child process, and can only be changed by fully stopping the server and then starting it again. ...

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• ab - Apache HTTP server benchmarking tool - Apache HTTP Server
• prefork - Apache HTTP Server
• mod_logio - Apache HTTP Server

... Abstract Replace a marker in a string with a formatted double precision value. ... Brief_I/O VARIABLE I/O DESCRIPTION -------- --- -------------------------------------------------- in I Input string. marker I Marker to be replaced. value I Replacement value. sigdig I Significant digits in replacement text. format I Format: 'E' or 'F'. lenout I Available space in output string. out O Output string. ... The first occurrence of marker in the input string is to be replaced by value. ... The value was #...

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• Mode = ACCUM Config = STIS/CCD
• CSPICE Routines: BODVRD_C
• CSPICE Routines: BODVCD_C

System parameters on Digital UNIX . ... Digital and Cray use the number of bytes as the KIND -parameter. ... LOGICAL Default byte word KIND number = 4 1 4 LOGICAL Default double quad KIND number = 4 8 16 INTEGER int15 int31 int63 KIND number = 2 4 8 digits = 15 31 63 radix = 2 2 2 range = 4 9 18 huge = 32767 2147483647 9223372036854775807 bit_size = 16 32 64 REAL single double quad KIND number = 4 8 16 digits = 24 53 113 maxexponent = 128 1024 16384 minexponent = -125 -1021 -16381 ...

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• SunSoft
• Specifications
• Summary of Fortran 77 statements

This document describes how number input can be given to tasks which request numbers from Hermes. ... list selection The following constants are implemented: pi 3.14159.... c speed of light (SI) h Planck (SI) k Boltzmann (SI) g gravitation (SI) s Stefan-Boltzman (SI) m mass of sun (SI) p parsec (SI) BLANK Universal undefined value The following mathematical functions are implemented: abs(x) absolute value of x sqrt(x) square root of x sin(x) sine of x asin(x) inverse sine ...

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• TPMODE
• casacore: casa::Dummy_Constants_class Class Reference
• Package: t

... This chapter discusses values that JavaScript recognizes and describes the fundamental building blocks of JavaScript expressions: variables and literals. ... So, for example, you could define a variable as follows: . var answer = 42 And later, you could assign the same variable a string value, for example, . ... These are fixed values, not variables, that you literally provide in your script. ... A string literal is zero or more characters enclosed in double ( " ) or single ( ' ) quotation marks. ...

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• ab - Apache HTTP server benchmarking tool - Apache HTTP Server
• worker - Apache HTTP Server
• Mean astrophysical parameters from LEDA

... There may be a need for binning the values as a typical observation of 40ks will either produce many pages or too many points per page to be useful if the number of columns requested is more than about 20. ... It may be useful to run a separate task like evselect to bin the data BEFORE running hkauxplot. pgplot currently creates it's own y-axis scales. ... While this task supports plotting EPIC and OM housekeeping and auxiliary files, it is not currently requested that they do so. ...

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• Algorithm

... File format . ... The p12mProg is the AO control program for the 12 meter telescope. ... the time from the tick, till when we complete the status read from the device. ... P12M_STAT_BLK struct (read from controller via group read at tick) . ... azimuth master 32bit status word . ... dbl . ... azimuth error read from controller. ... azimuth velocity read back from controller deg/sec . ... elevation position read back from controller. stBlk.elErr_D . ... elevation velocity read back from controller . ...

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• was hdr
• wst idl routines
• WAPP File Format Page

... In the above example, the second region uses the global coordinate system (PHYSICAL by default). ... Supported systems include: name description ---- ----------- PHYSICAL pixel coords of original file using LTM/LTV IMAGE pixel coords of current file FK4, B1950 sky coordinate systems FK5, J2000 sky coordinate systems GALACTIC sky coordinate systems ECLIPTIC sky coordinate systems ICRS currently same as J2000 LINEAR linear wcs as defined in file In addition, two mosaic coordinate ...

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• Mapping Pixel Values to Screen Intensity
• A matrix of tweets from #AAS225
• A quick look at tweets about JWST@SXSW

... There are number of features that can be set by the user in the Sparkle Dialog box. ... The Sparkle plug-in computes the luminosity (level of whiteness) of each pixel in the image (the user can see this when the progress window labeled Generating luminosity array... is displayed). ... The threshold value is currently a slider/text field pair which have a precision of .0001. ... Like the Threshold value, the Flare Intensity has both a slider and a text input field for specifying its value. ...

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• Authentication Options
• FTS Dictionary Example
• Number of Supernovae discovered by amateurs since 1957.

... They are the offset in arcseconds for the x and y inst plane offset, the exposure time in seconds, and the number of exposures at each position. ... A point about offsets should be made here. The dither program uses absolute instrument plane offsets, so you should use object plane offsets to center up on the chip so that the script starts from where you centered up. INST and OBJ offsets are independent so an object offset will not be zeroed out by and inst plane offset, just added to it. ...

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• TCC UDP Packets
• Guider Mechanical Commands
• DIS Commands

... Arithmetic Functions . Random Numbers . String Conversion . Searching and Sorting . ... There are 4 basic integer functions: . int abs(int number); long int labs(long int number); div_t div(int numerator,int denominator); ldiv_t ldiv(long int numerator, long int denominator); . ... In practice no functions produce truly random data -- they produce pseudo-random numbers. ... The stdlib.h provides 2 useful functions to perform general searching and sorting of data on any type. ...

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• LWN: Driver porting: miscellaneous changes
• Mathematics: <math.h>
• comedi_do_insn

NAME ab - Apache HTTP server benchmarking tool SYNOPSIS ab [ - k ] [ - i ] [ - n requests ] [ - t timelimit ] [ - c con- currency ] [ - p POST file ] [ - A Authenticate username : password ] [ - P Proxy Authenticate username : password ] [ - H Custom header ] [ - C Cookie name = value ] [ - T content - type ] [ - v verbosity ] [ - w output HTML ] [ - x table attributes ] [ - X proxy [:port] ] [ - y tr ... Default is no KeepAlive. - i Use an HTTP 'HEAD' instead of the GET method. ...

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• Apache module mod_log_common
• Apache module mod_vhost_alias
• Apache module mod_unique_id

... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

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spectrum1d - compute auto- [and cross- ] spectra from one [or two] timeseries. spectrum1d [ x [ y ] file ] -S segment _ size ] [ -C ] [ -D dt ] [ -N name _ stem ] [ -V ] [ -W ] [ -bi [ s ][ n ] ] [ -bo [ s ] ] spectrum1d reads X [and Y] values from the first [and second] columns on standard input [or x [ y ] file ]. ... Units same as ypower. name _ stem .npower Power spectral density of the noise output. Units same as ypower. name _ stem .gain Gain spectrum, or modulus of the transfer function. ...

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• http://xray.sai.msu.ru/~ivan/gmt/man/xyz2grd.html
• http://xray.sai.msu.ru/~ivan/gmt/man/grdtrack.html
• http://xray.sai.msu.ru/~ivan/gmt/man/sample1d.html

... These values are functions of the geographical (geodesic) latitude and the height of the point above the sea level. ... The option also permits to solve the reverse problem — to calculate approximate values of observatory latitude and its height above the sea level depending on the introduced values of dxy and dz. ... It should be mentioned that low precision of dxy and dz for some observatories in the list maintained by MPC leads to negative value of height above the sea level for some of them. ...

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• ENGAMPLE
• Values of asteroid masses

... public class CurveFitter . ... static int . ... Field Detail public static final int STRAIGHT_LINE . ... public static final int POLY2 . ... public static final int POLY3 . ... public static final int POLY4 . ... public static final int EXPONENTIAL . ... public static final int POWER . ... public static final int LOG . ... public static final int RODBARD . ... public static final int GAMMA_VARIATE . ... public static final int LOG2 . ... public static double f (int fit, double[] p, double x) . ...

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• MaximumFinder (ImageJ API)
• Plot (ImageJ API)
• Wand (ImageJ API)

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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• SPECPSF (V1.00) --- May00 stecf.specres --- SPECPSF (V1.00)
• Procedure to handle Waiver Requests
• Los Cielos de Am , The darkest sky and the two galactic hemispheres

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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• SLITLESS (Oct97) --- ST_ECF --- SLITLESS (Oct97)
• POLIMPLOT (V1.00) --- April99 --- POLIMPLOT (V1.00)
• SONTHOFEN HOTELS

... Simulation Images . Simulations of convection in stars . Mach-numbers in a simulation of convection inтАж . ... Title: Mach-numbers in a simulation of convection in the sub-giant Eta Boo . Description: The mach-number is the local speed in units of the local sound speed, with values above 1 being super-sonic. ... Mach-numbers in a simulation of convection in the sub-giant Eta Boo The mach-number is the local speed in units of the local sound speed, with values above 1 being super-sonic. ...

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• pynifs.velfit
• pynifs.nifscube
• pynifs

... A measure of the success of the web-site is the annual number of distinct e-Visitors (DEVs) to Armagh, in fact the number of distinct hosts served by the Observatory's web-site. ... During 2003, the numbers of successful page requests (i.e. `hits') to files of all types on each of the three web-sites listed were 3,983,000 (7-month's data), 890,000, and 675,000 respectively, whilst an estimated 470,000 Distinct e-Visitors visited the three web-sites during the year. ... 80,000 . ... 134,000 . ...

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• Simon Jeffery's Software Store: TAP: mathematical functions
• Simon Jeffery's Software Store: TAP chemical functions
• Armagh Observatory