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1. Input and Output
. Next: Stream 1/0 Up: C Standard Library Functions Previous: File Manipulation . Stream 1/0 . Low level I/O . Dave.Marshall@cm.cf.ac.uk . Wed Sep 14 10:06:31 BST 1994
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Ссылки http://mavr.sao.ru/hq/sts/linux/book/c_marshall/section2_21_6.html -- 2.1 Кб -- 28.12.2007
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/sts/linux/book/c_marshall/section2_21_6.html -- 2.1 Кб -- 11.09.2010
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/sts/linux/book/c_marshall/section2_21_6.html -- 2.1 Кб -- 02.10.2012
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[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/sts/linux/book/c_marshall/section2_21_6.html -- 2.1 Кб -- 11.09.2010
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/sts/linux/book/c_marshall/section2_21_6.html -- 2.1 Кб -- 02.10.2012
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2. Astronomy HyperText Book: Stellar Evolution
... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...
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Ссылки http://zebu.uoregon.edu/textbook/se.html -- 4.8 Кб -- 16.12.1997
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3. Redirecting standard input and output
. Unix considers any device attached to the system to be a file. And that includes your terminal! . By default, a command treats your terminal as the standard input file from which to read in information. Your terminal is also treated as the standard output file to which information is sent from the command. This action can be changed by redirecting standard input and standard output from and to any other file. Redirecting standard input . Redirecting standard output . Appending standard output to a file .
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Ссылки http://comet.sai.msu.ru/UNIXhelp/commanz/cmd3.html -- 2.2 Кб -- 17.01.1997
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4. stantAloneFiltersPrograms
... Interim correlator, ri . ... The programs with "filter" in column 2 are filter programs that read from standard input and write to standard output. The filters are classified as to their data input and output types: . ... BtoB: binary input to binary output . ... Programs Table . ... scan an interim correlator datafile and output a summary of each scan in the file. corstripch . ... read an ainterim correlator or ri datafile and output each scan to a separate file (or a subset of scans). ...
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Ссылки http://www.naic.edu/~phil/software/filters.html -- 15.3 Кб -- 12.03.2013
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5. Optical constant database - Level: data
. Mg x Fe 1 -x S from Begemann et al. (1994) . Use our codes to transform the standard data files to another form. Back to paper page . Last modified: 12/09/98, V.I.
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Ссылки http://www.astro.spbu.ru/JPDOC/PAPERS/BEGEMAN.94/mgfes.html -- 2.6 Кб -- 19.11.2010
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6. Reduction without Standard Star
Next: Saving the Data Up: The Reduction Session Previous: Flat Field correction . In the scheme described in the previous Section, the correction for the blaze function and for the chromatic response is done using standard stars. When the input data sets do not include standard stars it is possible to correct for the blaze function using a model of this effect as described in Chapter . ... where input is the raw image, . command MERGE/ECHELLE output name order1,order2 NOAPPEND . ...
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Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node476.html -- 3.6 Кб -- 23.02.1996
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7. Standard Setup Files
Next: Examples of Setup Files Up: Setup Files Previous: Setup Files Contents . Over 200 standard setup files have been created, covering many of the normal modes of observing. ... These especially include precisely defined, and somewhat complex cases like the Mark III standard modes (although MarkIII went the way of the dinosaur long ago. ... v '' files: . These are setup files for VLBI observations using VLBA recording formats. ... These are setup files for Mark III observations. ...
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Ссылки http://www.atnf.csiro.au/people/Tasso.Tzioumis/sched/Standard_Setup_Files.html -- 9.1 Кб -- 10.04.2016
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8. http://xray.sai.msu.ru/~ivan/gmt/man/trend1d.html
trend1d - Fit a [weighted] [robust] polynomial [or Fourier] model for y = f(x) to xy[w] data. trend1d -F < xymrw > -N [ f ] n _ model [ r ] [ xy [ w ] file ] [ -C condition _# ] [ -H [ nrec ] ] [ -I [ confidence _ level ] ] [ -V ] [ -W ] [ -: ] [ -bi [ s ][ n ] ] [ -bo [ s ] ] trend1d reads x,y [and w] values from the first two [three] columns on standard input [or xy [ w ] file ] and fits a regression model y = f(x) + e by [weighted] least squares. ... E.g., a robust quadratic model is -N 3 r . ...
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Ссылки http://xray.sai.msu.ru/~ivan/gmt/man/trend1d.html -- 8.1 Кб -- 19.03.1999
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9. CHIANTI atomic database
... MNRAS, 264, 627, 1993 % observed energy levels (4-5,7-8,12,14): NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61, 1995. % observed energy levels (16-58): Mendoza , C., Kallman, T.R., Bautista, M.A., Palmeri, P., 2004 , A , 414 , 377 %Theoretical energy levels (1- 15): Gupta, G.P., Tayal, S.S., 1998, ApJ, 506, 464 %Theoretical ...
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Ссылки http://www.arcetri.astro.it/science/chianti/chianti_5.1/database/fe/fe_13d.html -- 5.2 Кб -- 15.09.2005
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10. OptInt PmWiki : PmWiki / Forms
OptInt PmWiki : Pm Wiki / Forms . ... Forms processing can be found in the Cookbook (see below). ... input text name value size= n :) (:input hidden name value :) (:input password name value :) (:input radio name value :) (:input checkbox name value :) (:input select name value label :) (:input default default-name default-value :) (:input submit name value :) (:input textarea name [=value=] rows= n cols= n :) (:input reset name label :) (:input file name label :) (:input image name "src" alt :) . ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/pmwiki.php/PmWiki/Forms?action=print -- 16.6 Кб -- 01.03.2014
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11. http://www.stsci.edu/documents/dhb/web/c31_wfpc2error.fm3.html
... At the operating temperature of -88 C, maintained after April 23, 1994, the WFPC2 CCDs have a low dark background, ranging between 0.002 and 0.01 e - /s/pixel. A relatively small number of pixels have dark currents many times the value. ... The combined file is obtained by using the superdark value for all pixels that appear normal in the weekly dark, namely, for which the dark current value in the weekly dark does not differ from the superdark value by more than 3 . ...
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Ссылки http://www.stsci.edu/documents/dhb/web/c31_wfpc2error.fm3.html -- 7.8 Кб -- 17.11.1997
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12. NIST Special Publication 500-223. A Framework for the Development and Assurance
NIST Special Publication 500-223 . A Framework for the Development and Assurance of High Integrity Software . ... The purpose of this document is to recommend a framework for the development and assurance of high integrity software. ... High integrity software, project management, software assurance, software configuration management, software development, software hazard analysis, software quality assurance, software verification and validation. ... 2 SOFTWARE DEVELOPMENT . ...
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Ссылки http://www.cplire.ru/rus/casr/os/3_9/5.htm -- 4.5 Кб -- 21.03.2016
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13. ASP: Contents, Sep/Oct 1994
home publications > mercury . SEARCH ASP SITE: Match ALL words Match ANY word . ... ASP Conference Series . ... IAU Publications . ... Publications of the ASP (PASP) . ... Astronomy Beat . ... Mercury Magazine Contents . ... September/October 1994 . ... The Roots of Astrology , by Michael M. De Robertis and Paul A. Delaney . ... The standard response -- adding science education -- isn't enough. ... Starting virtually from scratch, astronomy proponents are building an astronomy education program. ...
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Ссылки http://www.astrosociety.org/pubs/mercury/9405/contents.html -- 21.6 Кб -- 20.04.2012
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14. http://www.adass.org/adass/proceedings/adass00/reprints/O3-03.pdf
... VSIPL and OpenMP are two open standards for portable high performance computing. ... Image processing is one of the main areas where VSIPL and OpenMP can have a large impact. Currently, a large fraction of image processing applications are written in the Interpreted Data Language (IDL) environment. The aim of this work is to demonstrate that the performance benefits of these new standards can be brought to image processing community in a high level manner that is transparent to users. ...
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Ссылки http://www.adass.org/adass/proceedings/adass00/reprints/O3-03.pdf -- 138.2 Кб -- 29.05.2001
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15. http://www.apo.nmsu.edu/arc35m/Instruments/ARCTIC/Development/ImagerPDR/LakeshoreTempControllerFamily.pdf
Lake Shore Temperature Controllers Adiabatic demagnetization refrigerators (ADRs) (50+ mK) Dilution refrigerators (DRs) (10 100 mK) Closed cycle refrigerators ... -4 K) Simple Dewars, LN cryostats ( 4.2 K) Description Application focus Standard number of sensor inputs (optional) Nominal low temperature capability (with appropriate sensor) Pumped He-3 systems (300 mK) Pumped He-4 systems (1.4 K) FlowHe-4 cryostats (4.2 K) Target ...
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Ссылки http://www.apo.nmsu.edu/arc35m/Instruments/ARCTIC/Development/ImagerPDR/LakeshoreTempControllerFamily.pdf -- 1153.3 Кб -- 05.12.2013
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16. The future of ISDN
... Most of the interesting R being done is in the B-ISDN world, and in the world of applications. ... The set of interoperability standards referred to is called National ISDN . The standardizing of applications is really separate from the ISDN standards themselves, but these applications will be important to the future success of ISDN. Currently research is being done into ??? vidphones, low-res voice, high-res sound, There is still a great deal of work being done here. ...
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Ссылки http://hea-www.harvard.edu/~fine/ISDN/future.html -- 2.7 Кб -- 01.10.2012
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17. Input Files
... event list files (one per CCD/node and per exposure), straight from the ODF. auxiliary files (one per exposure), straight from the ODF. offset/variance files (one per CCD/node and per mode), straight from the ODF. optionally, HK GTI files with STDGTI extension (one per exposure, from tabgtigen ). Their names must be standard ODF names ending in ``HKGTI.FIT'' ( i.e. HK as CCD/node number). ... optionally, bad pixels files with BADPIX extension (one per CCD/node and per instrument). ...
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Ссылки http://xmm.vilspa.esa.es/sas/5.4.1/doc/emchain/node13.html -- 4.0 Кб -- 10.01.2003
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18. http://www.gao.spb.ru/russian/psas/ffk2013/tfiles/Karshenboim_ffk2013.pdf
... The lines ( ) are equations: e.g., theoretical expressions for h/M, the Lamb shift, .. Some data are measured, a lot are derived: mp [kg], me [Mev/c2], .. ... for a `theoryґ for QHE steps rational universal relation to Needs for a `theoryґ for QHE steps rational universal relation to h block known from block input : h e NA h·NA h/me output me µB h block h block h block : the most important da t a h block : the most important da t a watt ballance Avogadro ...
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Ссылки http://www.gao.spb.ru/russian/psas/ffk2013/tfiles/Karshenboim_ffk2013.pdf -- 1352.2 Кб -- 25.11.2013
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19. recommended DFS development tools
DFS Department . Standard and recommended development tools . ... This tool is available on request from Helpdesk (except for the following machines: dfs3, dfs4 and dfs5, for which you have to contact Carlos ). ... Source Navigator IDE is recommended as a source code analysis and navigator tool for C, C++, Java, Tcl, [incr Tcl], FORTRAN and even COBOL on Linux:. ... webcheck is the DFS standard tool for archiving/retrieving DFS documents, web pages, Release Notes, schedules and ToDo lists. ...
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Ссылки http://www.eso.org/projects/dfs/team/QA-recom-dev-tools.html -- 15.5 Кб -- 04.12.2006
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20. Spectrum v1 - Input Syntax
The main input to SPECTRUM has been changed to allow a more flexible definition of some of the many options and to enable the elements of the code to be used in a more versatile way. ... The strict formatting of these files makes them unintelligible and the addition of new data inputs, options, etc., difficult. For example the mode of operation currently depends on the sign of certain data inputs! ... For the time being, both old and new style input will be recognised. ...
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Ссылки http://star.arm.ac.uk/~csj/software_store/guide/spectrum_v1.html -- 2.9 Кб -- 02.06.2003
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