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1. Creating an SCCS file
. To place files under the control of SCCS use the command: sccs create filename(s) . For each filename given as an argument sccs create does the following: . filename is moved to ,filename . a history file s. filename is created in the SCCS subdirectory . a "read only" copy of the initial version of the file is made by sccs get . You can use the ls command to check that the history files have been created. ls SCCS . Now you can remove the ,filename files: rm ,* .
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/UNIXhelp/utilities1/sccs_put3.html -- 2.3 Кб -- 17.01.1997
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2. Creating a swap space
Next: Using a swap space Up: Memory Management Previous: What is virtual memory? A swap file is an ordinary file; it is in no way special to the kernel. ... After you have created a swap file or a swap partition, you need to write a signature to its beginning; this contains some administrative information and is used by the kernel. ... Note that the swap space is still not in use yet: it exists, but the kernel does not use it to provide virtual memory. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/sag-0.4/node61.html -- 6.5 Кб -- 04.05.1997
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3. The File Life Cycle
The File System . This section describes how you can create new files, copy existing files, and delete obsolete files. ... RENAME to change the name of a file. ... Files can be created in several ways: text can be entered from the keyboard via the CREATE command, an editor can create a file, as can a running program, and files can be copied from other directories. ... To delete obsolete files, use the DELETE command followed by a file name or file name template (wildcards). ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/documents/system-docs/vms-guide/html/VUG_22.html -- 9.0 Кб -- 01.11.1995
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4. Creation of Sky Correction Frames
Next: Illumination Corrected Flat Up: Additional Processing Previous: Sky Illumination Corrections . For creation of one or more sky illumination correction frames the command ( SKYCOR/CCD ) is available. ... After this calibration step, the command will smooth the reduced sky frame(s) to create the final sky illumination frame(s). ... After the illumination frame has been created, one can multiply the original flat field by the illumination frame, resulting in an adjusted flat field. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node58.html -- 5.9 Кб -- 23.02.1996
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5. Creating a new sytem call: solution
The HyperNews Linux KHG Discussion Pages . Forum: The Linux Kernel Hackers' Guide . Re : Problem creating a new system call . ... From: C.H.Gopinath < gopich@cse.iitb.ernet.in > . ... If you want the data to be displayed on the stdout use sys_write(1,ptr,len); where ptr is the string to be displayed and len is its length. Using this you can check your sys call is created or not. ... I tried to assign and print a string in the system call. ... Kernel Debuggers for Linux by sauru . ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/doc/library/linux/khg/HyperNews/get/khg/135/1.html -- 3.5 Кб -- 23.03.2000
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6. CREATE FULLTEXT CONFIGURATION
... CREATE FULLTEXT CONFIGURATION -- create full-text configuration . CREATE FULLTEXT CONFIGURATION cfgname PARSER prsname [ LOCALE localename ] [ AS DEFAULT ]; CREATE FULLTEXT CONFIGURATION cfgname [ { PARSER prsname | ... PARSER . ... LOCALE . ... Create new configuration test with default parser and ru_RU.UTF-8 locale. CREATE FULLTEXT CONFIGURATION test PARSER default LOCALE 'ru_RU.UTF-8'; =# \dF+ test Configuration "public.test" Parser name: "pg_catalog.default" Locale: 'ru_RU.UTF-8' Token | ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/~megera/postgres/fts/doc/sql-fts-createcfg.html -- 10.1 Кб -- 13.04.2008
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7. Recreating Einstein Level One Processing Exposure Masks and Background Maps in
... This paper describes the main algorithms used by the Einstein Level One processing to create the exposure masks and the background maps for Einstein IPC images, and how these algorithms were recreated in the IRAF environment. Our goal was to recreate the algorithms used by the Level One Processing to create exposure masks and background maps for Einstein Image Proportional Counter (IPC) data (cf. sections 2.5 and 2.7 of Harnden et al. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/vanstoned.html -- 11.6 Кб -- 03.11.2000
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8. Creating reconstruction image and background image from an input source list
... If the parameter withinputlist is set to ``true'', the reconstruction and/or background image will be created using source parameters from an input source list. ... Use parameters makerecon and savebkgrnd to specify which of the output images you want to create. Only sources originally detected at scales up to maxscale will be used for to calculate the images. The value of maxscale will also control the scale of the kernel used to filter the background image. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/ewavelet/node9.html -- 3.8 Кб -- 01.07.2008
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