Modules | ... Apache HTTP Server Version 2.4 . ... Cookie based session support . ... session_cookie_module . ... The session modules make use of HTTP cookies, and as such can fall victim to Cross Site Scripting attacks, or expose potentially private information to clients. ... Name and attributes for the RFC2109 cookie storing the session . ... The SessionCookieName directive specifies the name and optional attributes of an RFC2109 compliant cookie inside which the session will be stored. ...

... Common options . All SAS tasks support the following command line options: . ... If the task uses the ODF Access Layer ( oal ) the following command line option is recognized as well: . ... odf odf . ... odf can be the name of an ODF summary file as created by the task odfingest or merely the name of a directory containing one. ... All tasks may have additional parameters in a parameter file, that can be set on the command line (more information can be found in package param ). param = value . ...

minmax - Find extreme values in data tables minmax [ files ] [ -C ] [ -H [ nrec ] ] [ -I dx [/ dy ] ] [ -M [ flag ] ] [ -: ] [ -bi [ s ][ n ] ] minmax reads its standard input [or from files] and finds the extreme values in each of the columns. It recognizes NaNs and will print warnings if the number of columns vary from record to record. ... C Report the min/max values per column in separate columns [Default uses <min/max> format] -H Input file(s) has Header record(s). ...

All existing data are plotted. ... Ion flux (VDP) - only solar wind and magnetosheath measurements are included (all meaningful measurements). Ion composition (PROMICS) data are available up to June 1996. ... Notations of the plot's axes are briefly explained in the plot header. ... When spacecraft attitude data are delayed, Y and Z components of magnetic field and plasma bulk velocity vectors can not be determined and are substituted by fill values. ...

Information is available for the following topics: . ... STIS Imaging . ... NICMOS . Flanking Fields . ... 2] (11/24/98) In the Version-1 data (11/23/98) there was an error in the G230L wavelength scale, introduced in the last step of the data reduction. ... 3] (11/24/98) Photometric zeropoints : There remains some significant uncertainty in the absolute photometric calibration of the NICMOS HDF-South images, with zeropoints for some bands uncertain at roughly the 10% level. ...

Modules | ... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Modules . ... Source File: . ... Because Apache for Windows does not have the Configure program of Apache for Unix, the module's source file must be added to the ApacheCore project file, and its symbols must be added to the os\win32\modules.c file. The second way is to compile the module as a DLL, a shared library that can be loaded into the server at runtime, using the LoadModule directive. ...

... printhdrV - print datataking headers in ASCII (ao) printhdrV [ -s ] . printhdrV is a program to convert ao datataking headers from binary to ASCII, format them with labels, and then output this data to the standard output. ... Arecibo datataking records contain a header followed by the data. ... Only output the standard header section. printhdrV can be used in conjuction with the stripVme (1l) and grep (1) programs to dump the headers of datataking tapes to the screen or a file. ...

fitshdr - FITS-file headers manipulation tool fitshdr [options] [FITSfile_name] . ... fitshdr [options] --edit FITSfile_name . ... If You want to modify headers of FITSFILE using new FITS-header lines from HEADER file (or from stdin), You have to use this option (You can skip this option, if -H or --header option is used). ... Empty header lines are not displayed (in 'dump' mode only). --line-offsets . ... In 'dump' mode: file offset will be displayed for each header line. --no-line-offsets . ...

... User Guide ] Task: fits Purpose: Conversion between Miriad and FITS image and uv formats Categories: data transfer FITS is a Miriad task that converts image and uv files both from FITS to Miriad format, and from Miriad to FITS format. ... References: For a description of the standard, see http://fits.gsfc.nasa.gov/fits_home.html Key: in Name of the input file (either a FITS or Miriad file name, depending on OP). ... Key: out Name of the output file (either a Miriad or FITS file name, depending on OP...

Next: List of PROS and Up: PROS USERS GUIDE Previous: Glossary . ... Available from SAO. ... The IRAF Data Reduction and Analysis System. ... File Structure and Formats of Processed Einstein Data [G. Fabbiano and J. McSweeney] - Details of the structure of the Einstein data files. ... User Manual for SAOimage [M. VanHilst] - Available from SAO. *documents so indicated are also available as compressed postscript files in subdir /pub/pros/docs of SAO anonftp. ftp sao-ftp.harvard.edu . ...

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. ...

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. ...

... Stellar Evolution . Nucleosynthesis in Stars . The Evolution of Star Clusters . JAVA Physics Lab . Alternative Energies Class . Steve Kevan's Physics 251 Class . ... Talk on Solid State Physics of CCD detectors . Talk on Cosmological Issues . ... Digital Spectra of Stars . NETexperts E-mail List . The Electronic Universe Project e-mail: nuts@moo.uoregon.edu ...

NAME ABbuilder - DFO data organization tool SYNOPSIS ABbuilder <options> where <options> are: --raw-dir directory containing raw data --cal-dir directory containing calib data --cal-ldir directory containing symbolic links to calib files --cal-list mcalib list --vcal-dir directory containing virtual products --pro-dir where pipeline products are created --ab-dir where association blocks are created --oca-rul file containing OCA rules --instrume instrument --date YYYY-MM-DD --mode { CALIB | ...

... One possible application of a solar sail is a spacecraft to warn Earth of approaching interplanetary disturbances and shocks. ... Spacecraft that can provide such a warning are currently stationed at (or near) the Lagrangian L1 point , between the Earth and the Sun--at about 4 times the distance of the moon and 1/100 times that of the Sun. ... Because of the greater distance from Earth, the Earth's pull there is weaker, not enough to make the spacecraft match the Earth's motion around the Sun. ...

... This command specifies the default delay to be used under these circumstances. ... This command configures a trap receiver at the given host address and port number for sending messages with the specified local interface address. ... While such monitor programs may also request their own trap dynamically, configuring a trap receiver will ensure that no messages are lost when the server is started. setvar variable [ default ] . This command adds an additional system variable. ...

I. Installation . ... AMPLE package distributive (created with program InstallShield for Microsoft Visual C++) has been downloaded on FTP server of IAA RAS as archive Ample.zip. ... Note: If the window "file download" appears, select Open... switch button, then press OK button. ... The shortcut for AMPLE will be linked with this folder, and auxiliary files will be created here during AMPLE work. ... When running AMPLE all auxiliary and new configuration files are created in the WORK folder. ...

. This section warns you against using the command in a way that might cause you problems.

This diagram illustrates a frame-like layout with 'position: fixed'. The illustration shows a four-panel frameset. The top panel ("header") covers the entire width of the frameset and takes up 15% of the vertical space. ... To the right of the sidebar and below the header is the "main" area, whose dimensions are computed based on remaining available space. Finally, at the bottom, the "footer" area is 100px high and covers the entire width of the frameset. ...

Allows you to specify the magnitude, proper motion, etc. of the object. ... Mag : magnitude of object. ... Obs Date : date of observation; used for correcting proper motion and radial velocity. ... PM RA/Long : proper motion in RA or Longitude, in arcsec/century. ... Warning: like all option panels, this one must be visible for its settings to have any effect. ... Defaults: restores this panel to its default values (the same values that will be used if you slew with this panel closed). ...