... Procedure . ... Wind Baffle Pendant Control, located in the 2.5m enclosure. Spreader Bar for wind baffle counterweights, located behind the Machine shop. ... Wind baffle frame tied to eyebolt in floor. ... Move the inner white wind baffle counterweight from the temporary mounting blocks at the front of the wind baffle frame to the standard location at the back. ... Rig the secondary truss to the overhead crane using a large shackle and 4 long nylon straps (load capacity of 1000 Lb. each). ...

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• Procedure to Install the 2.5m Wind Baffle
• SDSS M1 Mechanical Collimation
• APO Home Page

... SPICE User's Guides . brief - User's Guide for BRIEF, a utility program that allows you to summarize the ephemeris contents and coverage for one or more SPK files. ? ... commnt - User's Guide for COMMNT, a utility program that is used to add comments, extract comments, read comments, or delete comments in SPICE SPK, CK and EK files. ? ... tobin - User's Guide for TOBIN, a command line utility program that converts transfer format SPK, CK and EK files to binary format. ? ...

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• CSPICE Routines: SCE2C_C
• CSPICE Routines: SCE2T_C
• CSPICE Routines: NEARPT_C

Next: Plotting Up: Polarisation Previous: Polarisation . Currently the receiver position angle is not read from the RPFITS file and a position angle of zero is assumed. ... It is possible that there is a phase offset between polarisation which will effect the phase of the cross polarisation correlation, and so give rise to spurious polarisation. rotate_xyphase can be used to correct for this error. ... ASAP> scans.rotate_xyphase(10.5) # Degrees . ...

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• The Parkes 21cm Multibeam Project
• Satellite Tracking
• casacore: casa::MMapfdIO Class Reference

The vertex software has encoder corrections that can be interactively modified via the ocu or lcu interface. ... When adding a correction, the display position includes the correction. Preset mode works fine with the correction (eg. start at 270, add correction=1deg, display reads 271, preset to 270 moves the telescope be 1 degree). I think that program track mode works differently with the offsets.. mainly because we had an offset of 1 degree for 5 months and we could still see sources. ...

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• patriot 12 meter telescope
• wst idl routines

... Once "point" is read, assumes all the following x,y coordinates are points. ... Program asc2dxf c reads set of x,y coordinates and writes a .dxf file for aperture plate. character*4 xop1,xop2 character*12 outfile 1 format ( 1h0 /7hSECTION/1h2/8hENTITIES/ 1h0 ) 2 format (6hCIRCLE/1h8/1h1/2h62/1h3) 3 format (4hLINE/1h8/1h1/2h62/1h3) 4 format (5hPOINT/1h8/1h1/2h62/1h3) 5 format (2h10/5h43.00/2h20/5h43.00/2h30/5h0.000/2h40/5h43.00/ 1h0 ) 6 format (2h10,/,f6.3,/,2h20,/,f6.3,/,2h30/5h0.000) 7 ...

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... It interpolates the grid at the positions in the table and writes out the table with the interpolated values added as a new column. A bicubic [Default] or bilinear [ -Q ] interpolation is used, requiring boundary conditions at the limits of the region (see -L flag option). xyfile This is an ASCII [or binary, see -b ] file where the first 2 columns hold the (x,y) positions where the user wants to sample the 2-D data set. ... Default is 2 input columns]. -bo Selects binary output. ...

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• http://xray.sai.msu.ru/~polar/xmgr/points.html
• http://xray.sai.msu.ru/~ivan/gmt/man/fitcircle.html
• http://xray.sai.msu.ru/~ivan/gmt/man/trend1d.html

... Positions in 2000 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2001 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2002 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2003 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2004 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . ...

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• IAJ: Subscription Form
• Armagh Observatory

... In more detail, the task requires as main input a table in a data set which contains a column with times in XMM MET (Mission Elapsed Time) frame[1]. ... Parameter Mand Type Default Constraints withtable yes boolean true Whether to convert ta- ble in a dataset should be set to true if a table containing events to correct has been speci ed and to false otherwise. table yes string name of existing table a speci er which must point to a table in a data set. ...

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• http://xmm.vilspa.esa.es/sas/7.0.0/doc/earthbarycen.ps.gz
• http://xmm.vilspa.esa.es/sas/6.0.0/doc/earthbarycen.ps.gz
• http://xmm.vilspa.esa.es/sas/6.1.0/doc/earthbarycen.ps.gz

... Activity 3: Measuring the Position of the Sun in the Sky . Purpose: To give students the opportunity to measure the position of the Sun in the sky using simple tools and methods. ... Alternatively, you may have students devise their own methods of relative measurement and apply them to measuring the position of the Sun in the sky. ... Rangi is the sky, and when the Sun is near Rangi's head it is summer in New Zealand. ... Read the Maori story to students. ... back to Teachers' Newsletter Main Page ...

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... These HTML pages can be downloaded from SET.GMD.DE (/pub/misc/XFree86OS2/html) by FTP. This is XFree86 for OS/2, version 3.3.6 You don't have to download all files; just get the marked required files first, and then read the files and decide what you further need. ... Latest Information required (LATEST.OS2) . ... There are two flavours available, the full server and the small server which does not have the seldomly used PEX, XI, XIE extensions built in. 8514 server, full small (X8514.zip) . ...

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• Adding Variables to CONFIG.SYS
• Not so well documented Device Helpers in OS/2

Apache 1.1 and earlier let modules handle POST and PUT requests by themselves. The module would, on its own, determine whether the request had an entity, how many bytes it was, and then called a function ( read_client_block ) to get the data. ... This step also sends a 100 Continue response to HTTP/1.1 clients, so should not be called until the module is *definitely* ready to read content. (otherwise, the point of the 100 response is defeated). ... Finally, call ap_get_client_block in a loop. ...

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• Compiling Apache for Microsoft Windows

... The measurements themselves should be stored in a column with the label SIGNAL. ... Programs will expect that SIGNAL represents the integration of the photon flux for the exposure time given in the EXPTIME column (see section ). ... In that case, the column label should be RAWMAG; see Table . Programs will expect RAWMAG to be the usual negative logarithms of intensities; that is, RAWMAG values only use EXPTIME in determining weights. ...

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• Reading FITS
• Helpful Hints
• Initialisation of the Keywords

... comedi_dio_read -- read single bit from digital channel . ... int comedi_dio_read (comedi_t * device, unsigned int subdevice, unsigned int channel, unsigned int * bit); . The function reads the channel channel belonging to the subdevice subdevice of device device. The data value that is read is stored in the location pointed to by bit. This function is equivalent to comedi_data_read(device,subdevice,channel,0,0,bit). ... Return values and errors are the same as comedi_data_read(). ...

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• LWN: Using read-copy-update
• Stream 1/0
• Advanced Pointer Topics

Modules | ... Apache HTTP Server Version 2.4 . Apache > HTTP Server > Documentation > Version 2.4 > Developer Documentation . ... This is a first attempt at writing the lessons I learned when trying to convert the mod_mmap_static module to Apache 2.0. ... create per-server config structures */ . ... merge per-server config structures */ . ... 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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• LASG - Virtual private networks
• Procedures for Observations
• SSL/TLS Strong Encryption: How-To - Apache HTTP Server

Next: PointData manipulation Up: Accessing data files Previous: Loading tables Contents . Note that there are some procedures which package several tasks, e.g., get_pointdata includes loading of the configuration, scantable, etc., and the loading of point data for all scans. get_records Read raw data from HDS file. ... Note that configuration and table data must have been read prior to this call! get_rawdata ,[ file _char ] Compound procedure. ... Read scan data and auxilliary data from .cha file. ...

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• OIFITS reader
• ESO - ALMA
• Read configuration information, create tables, and load data

On 1 February 2002 this Mirror was upgraded from NVSSlist v2.10 to NVSSlist v2.17 . ... This form searches the source catalog produced by the NRAO/VLA Sky Survey (NVSS). ... Object name [optional] : . ... Search radius and verification halfwidth in arcseconds [Optional] : . ... Enter a list of positions to search: . ... The contents of the NVSS source catalog and the techniques used by NVSSlist to derive error estimates and other parameters are described here. ...

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• read_fits.c File Reference
• OptInt PmWiki : PmWiki / Upgrades
• exchange.h File Reference

... 32a. Early Solar Warning . ... Artist's rendering of solar sail. One such method is the use of a solar sail , relying on the pressure of sunlight. ... When the sail faces the Sun squarely, the pressure of sunlight counteracts the Sun's pull and only enables the satellite to circle the Sun in a slightly larger orbit. ... The starship is propelled by a huge solar sail, pushed by tight beams of light from lasers which are powered by sunlight and orbit the Sun. ... The solar sail home page . ...

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• Lagrangian Points
• The Lodestone
• Trigonometry--what it is good for?

... Artist's rendering of solar sail. One such method is the use of a solar sail , relying on the pressure of sunlight. ... When the sail faces the Sun squarely, the pressure of sunlight counteracts the Sun's pull and only enables the satellite to circle the Sun in a slightly larger orbit. ... The starship is propelled by a huge solar sail, pushed by tight beams of light from lasers which are powered by sunlight and orbit the Sun. ... The solar sail home page . ...

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• Trapped Radiation
• Lagrangian Points
• Magnetic Fields

... Class . ... ImageJ Plugin for reading an AVI file into an image stack (one slice per video frame) Version 2008-07-03 by Michael Schmid, based on a plugin by Daniel Marsh and Wayne Rasband Restrictions and Notes: - Only few formats supported: - uncompressed 8 bit with palette (=LUT) - uncompressed 8 16 bit grayscale - uncompressed 24 32 bit RGB (alpha channel ignored) - uncompressed 32 bit AYUV (alpha channel ignored) - various YUV 4:2:2 compressed formats - png or jpeg-encoded individual frames. ...

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• MaximumFinder (ImageJ API)
• University of Louisville Research Telescope at Mount Kent
• RandomAccessStream (ImageJ API)

Next: A box, to include Up: To produce a region Previous: To produce a region . select cursor and circle . When in the image window, the mouse now has a box shape with an arrow at the upper left corner. The mouse buttons act as follows: . LEFT - to move the center of the circle at the position of the arrow point. ... RIGHT - idle. center the circle at the point source by positioning the arrow point and clicking on the LEFT mouse button. A circle will appear at the arrow position. ...

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• The AstroStat Slog time series
• The AstroStat Slog breakdown point
• The AstroStat Slog datasets