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1. Graphical User Interface Example (3)
This third example shows how a Ggi plot window can be used. ... Or you can add a menu which enables the user to choose the graph's colour. The next example shows how cursor interaction can be added to the plot field. /* example3.c -XT */ #define NPTS 100 # include stddef.h # include math.h # include gipsyc.h # include cmain.h # include init.h # include finis.h # include userfio.h # include pgplot.h # include ggi.h static float a=1.0, b=1.0; ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/gipsy/pguide/gui-example3.html -- 6.7 Кб -- 17.01.2009
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2. Change history
... RDS . ... Calculates PSF correction for Timing/Burst. ... Rudimetary support has been added for spatial masks. ... 29 Oct 2002 . ... The Q.E. is applied for each detector map position. ... Added description for out-of-time event corrections. ... 03 Nov 2000 . ... Renumbered versions in Change History section. ... Updated description to reflect current functionality, specifically the detector map implementation and encircled energy correction. ... Added description for detector map feature. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.1.0/doc/arfgen/node3.html -- 15.6 Кб -- 15.11.2007
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3. NICMOS Proposing Example - 5
... NICMOS Proposing Example - 5 . ... Phase I Proposing . ... Real_Time_Justification: Calibration_Justification: Additional_ Comments : Fixed_Targets Target_Number: 1 Target_Name : HDF Alternate_Names: Hubble Deep Field Description: GALAXY,PROTOGALAXY Position: RA=12H 36M 49.40S +/- 0.02S,DEC=62D 10' 58.0 ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/nicmos/proposing/examples/1044.prop -- 19.6 Кб -- 11.04.2016
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4. Symbol Substitution in Command Procedures
Next: DO Loops Up: MIDAS Command Language Previous: Passing Parameters in . As mentioned before, the Monitor performs symbol substitutions on MIDAS command lines in the first pass by replacing symbol names in the command line with their current value. For character symbols just the string is put in; for symbols of other types the binary data are converted to ASCII using the formats specified in the SET/FORMAT command. ... Example 6, MIDAS procedure exa6.prg . ... WRITE/KEYWORD VAR/R/1/1 0. ! ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol1/node42.html -- 13.8 Кб -- 23.02.1996
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5. http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/reset.htm
... A reset button on an HTML form. ... Client-side object . ... JavaScript 1.1: added type property; added onBlur and onFocus event handlers; added blur and focus methods . JavaScript 1.2: added handleEvent method The HTML INPUT tag, with "reset" as the value of the TYPE attribute. ... JavaScript 1.0 blur() None The following example removes focus from the reset button userReset: userReset.blur() This example assumes that the button is defined as <INPUT TYPE="reset" NAME="userReset"> Reset.focus . ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/reset.htm -- 21.9 Кб -- 07.10.1999
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6. (Untitled)
To construct frequency distribution (histogram) of minor planets according to value of some element/ parameter/ function user should first select Elements item in menu bar and then Histogram in drop-down menu. ... User has possibility to save histogram or to print it using standard means. To save the file select File item in menu bar and then Save As... in drop-down menu. ... To print histogram select File item in menu bar and then take advantage of options Print Preview , Print Setup , Print . ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user4oqb.htm -- 4.2 Кб -- 10.04.2016
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7. Change of Binary Parameters: Mass, Semi-major Axis and Eccentricity
Next: Mass change Up: Evolutionary Scenarios of Binary Previous: Stellar Winds From Normal . As mentioned earlier, the duration of the binary evolutionary stage (say, I+I) is determined by the faster evolving component , where is the time each component spends at the corresponding evolutionary stage. ... Next, we should calculate the mass change for the slower evolving companion, the orbital semi-major axis and the eccentricity. Mass change . Semi-major axis change . ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node11.html -- 4.3 Кб -- 25.02.1997
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8. Example of changing a password with the passwd command
To change your password: passwd Old password: enter your current password New password: enter your new password Retype new password: re-enter your new password . Enter the command passwd and then respond to the prompts by entering your old password followed by your new one. ... The passwords will not appear on the screen as you type, to prevent other people from seeing them. If you make a mistake, the message Mismatch - password unchanged. is displayed and your password remains unchanged. ...
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/UNIXhelp/basics/basic3.1.html -- 2.3 Кб -- 17.01.1997
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9. Spectrum - control
... spectrum . ... nsource <n> : choice of source function (def: 3=Feautrier) . noptype <n> : choice of continuous opacity (def: 1=Kiel) . nhedat <nhedat> : choice of HeI data (BCS or Mon treal) (def: 1=BCS) . ... read_model <filename>: read model atmosphere in QUB/STERNE2 format . ... wavmax <w_max> : distance from line centre to compute . ... nvturb <n vt > : number of points in -dependent v turb . ... tau_exp <n> : increase resolution of optical depth scale by adding additional points . ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~csj/software_store/guide/spectrum_commands.html -- 10.8 Кб -- 03.06.2012
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10. Parameters
... IRAF supports two kinds of parameters, auto parameters and hidden parameters, which are treated differently. auto parameters are updated every time a task is run. ... Parameters for each task are contained in `parameter files' in the uparm sub-directory in `myiraf'. ... im > imhead.longheader=yes # explicitly setting <task.param>=<value> im > eparam imhead # Edit the parameter file to update one or more # parameters at the same time # see next section . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node8.html -- 5.0 Кб -- 01.10.2012
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11. Conformance: requirements and recommendations
... SGML . The text/html content type . In this section, we begin the specification of HTML 4.0, starting with the contract between authors, documents, users, and user agents. ... These recommendations are not normative and conformance with this specification does not depend on their realization. ... An HTML document is an SGML document that meets the constraints of this specification. ... A user is a person who interacts with a user agent to view, hear, or otherwise use a rendered HTML document. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~ustiansk/web/conform.html -- 12.1 Кб -- 24.04.1998
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/~vab/html.doc/html40/conform.html -- 12.1 Кб -- 24.04.1998
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12. ALTER FULLTEXT ... OWNER
... ALTER FULLTEXT .. OWNER -- change the owner of a full-text object . ALTER FULLTEXT { PARSER|DICTIONARY|CONFIGURATION } name OWNER TO newowner ; . ... The new owner of the full-text object. ... Then we change owner of the new dictionary. ... CREATE SCHEMA test; =# CREATE FULLTEXT DICTIONARY test.synonym LIKE pg_catalog."synonym"; =# SHOW search_path; search_path ---------------- "$user",public =# SET search_path TO test,public; =# ALTER FULLTEXT DICTIONARY synonym OWNER TO megera; . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/~megera/postgres/fts/doc/sql-fts-alterowner.html -- 5.1 Кб -- 13.04.2008
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13. Writing programs that use comedi and comedilib
Comedi Documentation . ... Right to the source: #include <stdio.h> /* for printf() */ #include <comedilib.h> int subdev = 0; /* change this to your input subdevice */ int chan = 0; /* change this to your channel */ int range = 0; /* more on this later */ int aref = AREF_GROUND; /* more on this later */ int main(int argc,char *argv[]) { comedi_t *it; lsampl_t data; it=comedi_open("/dev/comedi0"); comedi_data_read(it,subdev,chan,range,aref,&data); printf("%d\n",data); return 0; } . ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/sts/linux/comedi/doc/x94.html -- 8.9 Кб -- 28.12.2007
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/sts/linux/comedi/doc/x94.html -- 8.9 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/sts/linux/comedi/doc/x94.html -- 8.9 Кб -- 02.10.2012
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14. IKI SSC, INTMINS APRIL99
Modified 11 April 1999. The last modifications concerns to the new ground tracks selection on the base of the more wide list of the INSPIRE particpants. ... The range value was changed from 2 deg to 4 deg for the distance between lat/lon of the graund track and place of the INSPIRE members. Plots of predicted tracks under USA and Europe 11 April 1999 . April, 17, 1999 (USA) . April, 17, 1999 (EUR) . ... 11 April 1999 . ... place . ... Back to the IKI Satellite Situation Center (SSC) . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/vprokhor/intmins/april99.htm -- 8.0 Кб -- 11.04.1999
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/vprokhor/intmins/april99.htm -- 8.0 Кб -- 11.04.1999
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15. http://www.naic.edu/~emuller/icred
Some Documentation for the IDL ICRED . ... This is the system which recieves all command inputs. it decodes inputs and selects tasks, parses parameter inputs and also runs the 'go', 'list' and 'help' commands. It does no error checking, for example to see if the parameter inputs are sensible (e.g. it does not check if an x-range has been entered as 'chicken', rather than a more understandable range of say 10,20). 2) the task decoders: icred_<taskname>.pro . ... Other tasks or important commands: . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~emuller/icred -- 8.4 Кб -- 21.10.2004
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16. Theoretical Astrophysics
Subject, Problems and Objects of Theoretical Astrophysics. ... Stellar Photospheres, Their Features. ... Physics of Continuous Radiation Absorption in Stellar Photospheres. ... Continuous Radiation Absorption in Stellar Photospheres of Various Spectral Classes. Solar Type Photospheres. ... Characterisics of Absorption Lines. ... Interstellar Absorption Lines, Their Features. ... Physical and Dynamic Features of Interstellar Medium, Which Follows from Observations of Interstellar Absorption Lines. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/courses/teor_astroph_e.html -- 8.7 Кб -- 23.02.2005
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17. Command line interface to libAIR and water vapour column retrieval Bojan
... Bojan Nikolic web pages (r. 329) . ... Since version 0.12, libAIR comes with a simple command line interface to the routines which retrieve the water vapour and the phase correction coefficient. Currently only the very simplest model is supported, in which the all of pressure, temperature and water vapour column are free parameters, and they are inferred from the four observed water vapour radiometer readings. ... Command line interface to libAIR and water vapour column retrieval . ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/alma/libaircmdline.html -- 10.4 Кб -- 04.04.2016
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18. Phil Plait's Bad Astronomy: Misconceptions
... Bad Astronomy . ... I think I will break from my usual format of Bad Astronomy/ Good Astronomy by saying that the way we define seasons currently is not strictly bad, but I feel (in my opinion!) that it could be better. The definition of when the seasons begin is at the moment of solstice or equinox; that is, winter (in the north) starts on December 22 nd and summer starts on June 22 nd . ... Now imagine breaking up the Sun's 46 degree up-and-down yearly swing into 1 day intervals. ...
[ Сохраненная копия ]  Ссылки http://www.badastronomy.com/bad/misc/badseasons.html -- 24.7 Кб -- 09.04.2016
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19. POLIMODEL (V2.00) --- November00 --- POLIMODEL (V2.00)
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. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~jwalsh/softpol/polimodel.help.html -- 6.1 Кб -- 02.11.2000
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20. POLIMODEL (V1.00) --- April99 --- POLIMODEL (V1.00)
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. ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/impol/polimodel.help.html -- 6.1 Кб -- 06.06.2006
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