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1. tickadj - set time-related kernel variables
... The particular variables it is concerned with are tick , which is the number of microseconds added to the system time during a clock interrupt, tickadj , which sets the slew rate and resolution used by the adjtime system call, and dosynctodr , which indicates to the kernels on some machines whether they should internally adjust the system clock to keep it in line with time-of-day clock or not. ... Set the kernel variable tickadj to an internally computed "optimal" value. -t tick . ...
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Ссылки http://www.sai.msu.su/~er/xntp/tickadj.html -- 4.0 Кб -- 21.12.2007
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2. CSPICE Routines: VRELG_C
... Abstract Return the relative difference between two vectors of general dimension. Required_Reading None. ... Detailed_Input v1, v2 are two vectors for which the relative difference is to be computed. ndim is the dimension of v1 and v2. Detailed_Output vrelg_c is the relative difference between v1 and v2. ... Particulars This function computes the relative difference between two vectors of general dimension as defined above. ... Index_Entries relative difference of n-dimensional vectors . ...
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Ссылки http://www.stsci.edu/~sontag/spicedocs/cspice/vrelg_c.html -- 7.7 Кб -- 17.12.2005
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3. Pulsar Group PmWiki/Link Variables
... Summary: PmWiki group header. ... Summary:variables that control the display of links in pages:) (:Audience: admins (advanced):) . ... When enabled, causes PmWiki to use relative urls for page links instead of absolute urls. ... This array lists the order in which PmWiki looks for the page that you most likely are attempting to link to. ... Defaults to <a class='wikilink' href='\$LinkUrl'>\$LinkText</a> . ... The default is to add a '?' after the link text with a link to the page edit/create form. ...
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Ссылки http://www.atnf.csiro.au/people/pulsar/index.html?n=PmWiki.LinkVariables -- 22.0 Кб -- 01.03.2014
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4. EPIC Related CAL Routines
Next: CAL_getHKwindows Up: Routines of the Calibration Previous: List of CCF Components Contents . ... CAL_getHKwindows . Procedure . ... Used CAL State Variables . List of CCF Components used . CAL_getAUXwindows . ... CAL_getBoresightMatrix . ... CAL_rawXY2mm . ... CAL_mm2rawXY . CAL_rawX2chipX . ... CAL_chipX2rawX . ... CAL_getBadPixelList & CAL_getBadPixelMap . ... CAL_mosCTIcorrection . ... CAL_getmosOffset . ... CAL_mosgainCorrect . ... CAL_getEventPatterns . ... CAL_getEbounds . ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node44.html -- 17.9 Кб -- 20.09.2011
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5. OptInt PmWiki : PmWiki / Link Variables
OptInt PmWiki : Pm Wiki / Link Variables . ... When enabled, causes PmWiki to use relative urls for page links instead of absolute urls. ... The default is listed below. ... Defaults to <a class='wikilink' href='\$LinkUrl'>\$LinkText</a> . ... Links to https: secure pages: $IMapLinkFmt ['https:'] = "<a class='httpslink urllink' href='\$LinkUrl'>\$LinkText</a>"; . Links to PmWiki: InterMap shortcut: $IMapLinkFmt ['PmWiki:'] = "<a class='pmwikilink urllink' href='\$LinkUrl'>\$LinkText</a>"; . ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/pmwiki.php/PmWiki/LinkVariables?action=print -- 19.1 Кб -- 01.03.2014
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6. IDLINES: identifying spectral lines
... IDL procedure to display ; a) a region of spectrum , together with a fit , if supplied, ; b) positions and relative strengths (gf or W_lambda) of lines in ; common atomic spectra may be marked in the lower panel. ; c) lines of sleceted atoms are identified in the top panel ; ; Command arguments: ; specfile - character string - name of file containing spectrum (and fit ) ; assumed to be x,y file with 3- ... Assesses lines in linelist by the strength values "listfr". ...
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Ссылки http://star.arm.ac.uk/~csj/idl/IDL_idlines.html -- 4.6 Кб -- 05.05.2009
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7. Text attribute examples
My preferred browser is Netscape Navigator . ... Netscape Navigator lets the user select a comfortable base font size, but this can be reset for all or part of a page. ... As Alice ate the cookies, she felt herself grow bigger, and bigger, and bigger. ... Blinking text can be annoying, so use it sparingly. ... The onLoad attribute for the BODY tag lets you define an action that occurs when the document has finished loading. For example, onLoad="function1(); function2(); return false;" . ...
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Ссылки http://www.sao.ru/cats/~satr/JS/REF/text.htm -- 7.4 Кб -- 26.03.1998
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8. lsst.tcc: tcc.axis.instFromObs Namespace Reference
lsst.tcc љ 1.2.2-3-g89ecb63 . ... Namespaces . ... NamespaceљList . ... instFromObs . ... tcc.axis.instFromObs Namespace Reference . ... Compute instrument position from observed coordinates. ... position of target in observed coordinates (a coordConv.PVTCoord) . ... targInstXY: position of target in instrument coordinates (a tcc.base.ArrayPVT2) (deg) i.e. a position in instrument X,Y relative to inst.iim_ctr, the center of the instrument . ... list tcc.axis.instFromObs.__all__ = ["instFromObs"] . ...
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Ссылки http://www.apo.nmsu.edu/Telescopes/TCC/html/namespacetcc_1_1axis_1_1inst_from_obs.html -- 10.8 Кб -- 14.09.2015
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9. Chapter 11. Specifying OpenGL Environment Variable Settings
Chapter 11. Specifying OpenGL Environment Variable Settings . ... Several antialiasing methods are available and you can select between them by setting the __GL_FSAA_MODE environment variable appropriately. ... To see the available values for __GL_FSAA_MODE along with their descriptions, run: nvidia-settings --query=fsaa --verbose . The __GL_FSAA_MODE environment variable uses the same integer values that are used to configure FSAA through nvidia-settings and the NV-CONTROL X extension. ...
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Ссылки http://www.naic.edu/~phil/hardware/nvidia/doc/driverInstall/chapter-11.html -- 10.3 Кб -- 30.10.2009
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10. ASP: A Taste of Real Astronomy ? The ESA/ESO Astronomy Exercises
The ESA/ESO Astronomy Exercise Series 2 . The Distance to Messier 100 as Determined by Cepheid Variable Stars . ... The small variations in distance to the individual Cepheid variable stars in the Cloud are negligible compared with the much larger distance to the SMC. ... In this way Cepheid variable stars can be used as one of the 'standard candles' in the Universe that act either as distance indicators themselves or can be used to calibrate (or set the zero point for) other distance indicators. ...
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Ссылки http://www.astrosociety.org/edu/publications/tnl/57/realastro3.html -- 14.8 Кб -- 02.10.2012
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11. Access Control - Apache HTTP Server
... Directives | ... Apache HTTP Server Version 2.4 . ... Access control refers to any means of controlling access to any resource. ... Access control by host . ... If you wish to restrict access to portions of your site based on the host address of your visitors, this is most easily done using mod_authz_host . The Require provides a variety of different ways to allow or deny access to resources. ... The usage of these directives is: Require host address Require ip ip.address . ...
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Ссылки http://www.arcetri.astro.it/manual/fr/howto/access.html -- 13.8 Кб -- 19.11.2015
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12. Journal "Peremennye Zvezdy"
Peremennye Zvezdy", . ... 6, N 19 (2006) . ... Star Name: . ... Fourier-decomposition of the light curves shows frequency peaks at 1.55 c/d and its ?1.0 day aliases. ... V lightcurve and B-V, V-R C , V-I C colour index curves are shown, folded with the period of P=0.645 days. ... 2006, IBVS 5709 . ... Light Curve . USNO-B1.0 1305-0178165 relative V light curve and relative B-V , V-R C and V-I C colour index curves, from top to bottom, respectively, folded with the 0.645d period of the variation. ...
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Ссылки http://www.astronet.ru/db/varstars/msg/1214919 -- 11.5 Кб -- 26.02.2007
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13. RR LYRAE VARIABLES SUBSYSTEMS IN THE GALAXY, figures
... 2. (a) Metallicity function and relations between (b) metallicity and radial velocity, (c) metallicity and maximum distance from the Galactic plane,and (d)metallicity and variability period for RR Lyrae variables in the initial sample.The curve in the first graph is the maximum-likelihood approximation of the distribution using a sum of two normal curves with the indicated means,dispersions,and total numbers. ... next figure | privious figure . ...
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Ссылки http://ip.rsu.ru/~marsakov/paper6/p6fg2_1.htm -- 2.4 Кб -- 02.02.2007
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14. http://www.mso.anu.edu.au/~wood/lectures2009/Pulsation_1.pdf
ASTR 3007 - STELLAR PULSATION COMPONENT P e ter W o o d Research School of Astronomy & Astrophysics TOPICS COVERED · Main types of variable stars · Linear adiabatic pulsation theory => periods of pulsation · Linear non-adiabatic pulsation theory => stability - will a star pulsate? ... Here we see Cepheids and long-period variables (LPVs) (movies from Hartman: http://cfa-www.harvard.edu/%7Ejhartman/) WHY STUDY VARIABLE STARS? ... What could cause the pulsation period to vary from star to star? ...
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Ссылки http://www.mso.anu.edu.au/~wood/lectures2009/Pulsation_1.pdf -- 1998.4 Кб -- 26.03.2009
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15. Division of the Galaxy and Variable Stars
Rastorguev А.S. "Astronomical Distances" (Lecture course for postgraduates, 2009-2016) . Part 1. ... Trigonometric parallaxes of stars. Moving clusters distances. ... Photometric distances: general approach. Normal stars as "standard candles". ... Main Sequence fitting or distance scale of star clusters. ... Moving photospheres technique. Cepheid distance scale and P-L relations. RR Lyrae distance scale. ... Globular clusters luminosity function. ...
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Ссылки http://lnfm1.sai.msu.ru/~rastor/AD.HTM -- 3.1 Кб -- 31.03.2016
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16. http://www.issp.ac.ru/iao/2015/booklet/b10_ia15_p_en_a.pdf
... A star was observed at different zenith distances during one night at the Engelgardt's Astronomical Observatory in the program of atmospheric extinction study at blue. ... The determination of the star's brightness was performed with the method of photon counting. ... Variable star. ... The brightness of the variable star was measured occasionally during the other nights, and moments of maximal values of brightness (15.59m) were received on nights 25, the 2nd table. ... JD 2452805. ...
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Ссылки http://www.issp.ac.ru/iao/2015/booklet/b10_ia15_p_en_a.pdf -- 173.2 Кб -- 03.12.2015
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17. http://jet.sao.ru/jet/~goray/estimate/text.html
1) Find the variable star and the comparison stars marked in the map. 2) Seeing the the variable star, try to imagine its location in the brightness interval between the reference stars. 3) Looking at the specially prepared scale, try to reproduce the location of variable in the brightness scale from memory. ... The grades of arbitrary scale are marked relative to brightness intervals between the reference stars. ...
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Ссылки http://jet.sao.ru/jet/~goray/estimate/text.html -- 1.7 Кб -- 22.07.2005
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18. Multiwavelength Study of Mira Ceti-Type Variable Stars
... There are preliminary series of photometric and radio spectral observations of the above-mentioned stars, archival data on the light curves of the stars, results of the search for OH and H 2 O maser emission in IRAS point sources that possess the IR parameters similar to Miras. ... The aim is a detailed study of the maser emission variability. ... In 1996-1997, astronomical observations of Mira Ceti-type stars (miras) were carried out in three spectral ranges: optical, infrared, and radio. ...
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Ссылки http://comet.sai.msu.ru/~gmr/miras.html -- 13.9 Кб -- 25.11.2015
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19. Detection of Radio Transients and Variable Radio Sources Using the Archive Data
... During the analysis of the surveys carried out on RATAN-600, it was found that almost one fifth of the detected sources shows significant radio flux variations. ... We used the data from "Cold" radio surveys carried out with RATAN-600 in 1980-1994 to search for radio sources with significant flux variability. ... On possibility of detection of variable sources using the data of Cold surveys carried out on RATAN-600. ... Detection of Variable Sources Using the Data of "Cold" Surveys. ...
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Ссылки http://www.sao.ru/Doc-en/SciNews/2016/Zhelenkova/ -- 6.9 Кб -- 10.04.2016
[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/2016/Zhelenkova/ -- 6.9 Кб -- 10.04.2016
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[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/2016/Zhelenkova/ -- 6.9 Кб -- 10.04.2016
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20. Restrictions on the Scenario Parameters
... we show that the comparison between the calculated and observed numbers of the most ``fragile'' (from the point of view of the binary evolution scenario ) galactic binary types (such as X-ray low-mass X-ray binaries (LMXB), cataclysmic variables (CV), Be-stars with compact companions, relative number of visible binary radiopulsars with normal and compact secondary components) impose certain constraints on the feasible initial ... Phenomenological Kick Velocity . ...
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Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node41.html -- 6.6 Кб -- 26.02.1997
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