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1. User Parameters - Data Location & Beam Selection CentralProcessor 0.11
... CentralProcessor 0.11 documentation . ... The following parameters determine where the measurement sets are that hold the data to be processed. The default behaviour is to read the MS from the given Scheduling Block (SB) directory. ... Location (on galaxy) of the scheduling blocks. This is used when specifying SB numbers - the default is the standard location for BETA operation. ... These parameters determine which beams in the data to process. ... User Parameters - Pipeline & job control . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/askapsoft/sdp/docs/current/BETApipelines/DataLocationSelection.html -- 8.5 Кб -- 12.04.2016
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2. Parameters for EMOS 1
... HK file type: PeriodicHousekeeping [22 parameters ] ---------------------------------- FILTER_WHEEL string [E1257] FILTER_WHEEL_POSITION Uint16 [E1317] FILTER Uint16 [E1317] This parameter is translated as follows : Translator's name: EMOS1 Filter 0 = Closed 247 = CalThin1 267 = Thin1 514 = CalThin2 534 = Thin2 781 = CalMedium 801 = Medium 1047 ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/6.5.0/doc/odfingest/node8.html -- 8.2 Кб -- 15.08.2005
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3. http://www.stsci.edu/documents/dhb/webvol2/c16_hspcalib.fm3.html
... Computing the true count rates for digital data. ... The following equation is used to find the count rate. x = ( raw counts / sample time ) . ... True count rates for digital data are corrected by using the first equation for a point source and the second for an extended source. a = ( y - pre_amp - darkrate ) / ( highvolt x pt_effic ) . ... True photocurrents (count rates for analog data) are corrected by the first equation for point sources and the second equation for extended sources. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/documents/dhb/webvol2/c16_hspcalib.fm3.html -- 7.2 Кб -- 10.02.1998
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4. The main observational parameters
... Column 1 gives the object name from the Case or Markarian catalogs. ... For Markarian galaxies the errors of coordinates usually lie inside 2'' (Lipovetsky [ 1983 ]). Column 4 gives the eye-estimated apparent blue magnitudes according to the same sources. ... Other names of a galaxy we give in column 7. ... In column 3 we cite the original emission-line code of the galaxy for the strength of [O III ] doublet according to the Case catalog (s - strong, m - medium, w - weak). ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Laboratory/Publications/1997/CasePR/node7.html -- 10.4 Кб -- 10.01.1998
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5. Getting Started in Actor Prolog. Oil Production.
In this chapter we will consider an example of visual expert system written on the Actor Prolog language. ... There are a lot of methods of oil field bed stimulation that increase output of the oil production: thermal, physical-chemical, gas, microbiological, and others. ... Fig. ... The Top-Most diagram consists of three blocks: the "Describe parameters of hydrocarbon field" block, the "Check adaptability of existed methods of oil production" block, and the "Display solution" block. ... Gas methods. ...
[ Сохраненная копия ]  Ссылки http://www.cplire.ru/Lab144/start/e_oil.html -- 12.2 Кб -- 24.09.2007
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6. CONSTRICTOR parameters for astrometric reductions
Next: Coherent integration Up: Astrometry data reduction Previous: Introduction Contents . ... In order to increase the SNR for these data, we coherently integrate the complex visibility for typically 200 ms. The coherent integration is done using the COBRA procedure cohstrictor . In order to provide the necessary input file for this step, the following CONSTRICTOR parameters should be used. ... The .coh extension is standard for coherent integration. ... NumAv = 100. ... Pass on metrology data . ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~chummel/oyster/manual/node194.html -- 3.9 Кб -- 28.04.2015
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7. Your NED Search Results
... NED Home . ... Redshift: Between 0.150000 and 0.270000 . Include ALL Object Type: QSO Radio . ... Number of Essential Note) RA DEC Type km/s z Qual arcmin Refs Notes Phot Posn Vel/z Assoc Images 1 30000 0.228000 0.0 26 0 8 3 0 0 Retrieve 2 30000 0.181000 0.0 5 0 4 1 0 0 Retrieve 3 30000 0.171000 0.0 67 1 1 0 0 0 Retrieve 4 30000 0.260000 0.0 90 1 16 5 0 0 Retrieve 5 30000 0.163009 0.0 170 10 5 4 3 0 Retrieve 6 30000 0.245000 0.0 27 1 1 2 1 0 Retrieve 7 30000 ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~tghosh/list2.html -- 55.4 Кб -- 05.08.2001
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8. Initial parameters of compact stars
Next: Other parameters of the Up: The Model Previous: Initial binary parameters . As we only deal with initially massive binary systems (their primary's mass is higher than 10 ), which are capable of evolving off the main sequence during less than years, the compact stars left behind stellar evolution are (in the case of the most massive stars) NSs and BHs. ... For a NS belonging to a binary, the evolution complicates as the secondary star evolves: for example, (recycling), etc. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~polar/html/publications/apj/node4.html -- 8.4 Кб -- 21.06.1996
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9. http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/boolean.htm
... The Boolean object is an object wrapper for a boolean value. ... JavaScript 1.3: added toSource method . ... If value is omitted or is 0, -0, null, false, NaN , undefined, or the empty string ( "" ), the object has an initial value of false. All other values, including any object or the string "false" , create an object with an initial value of true. ... For Boolean objects and values, the built-in toString method returns the string "true" or "false" depending on the value of the boolean object. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/boolean.htm -- 16.3 Кб -- 07.10.1999
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10. Database of Optical Properties -- Level: subsubpage
Their dependence on the diffraction parameter x for several refractive indeces m=n+k i is given in the following figures: . Parameters . ... n =1.5, 2.5, 3.5; . ... fig . ... Their dependence on the scattering angle theta for several diffraction parameters x and refractive indeces m=n+k i is given in the following figures: . ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/staff/ilin2/DOP-old/2-24sm.html -- 5.3 Кб -- 19.11.2010
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11. (Untitled)
Following designations of elements/ parameters are used in AMPLE. ... mean anomaly . ... Node . ... Apart conventional orbital elements AMPLE gives possibility to calculate for each minor planet the following often used functions: . ... MOID . ... To calculate MOID user should order the name or the number of the major or minor planet through dialog. ... To calculate CT user should order the name or the number of the major or minor planet through dialog as it is proposed for MOID calculation. ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user8mge.htm -- 7.5 Кб -- 10.04.2016
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12. Fixing and Freeing Region Markers
Region markers can be moved, resized, rotated, zoomed, deleted, and can change geometric type. ... For example, markers placed on astronomical catalog positions should be fixed so that one cannot accidentally move them off the specified position. ... Parameters can be fixed using the fix option of the regions public access point (for fixing classes of markers) or by means of a fix keyword in the definition of an externally loaded marker. ... In the command: echo "regions fix all -position -size" | ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/RD/saotng/fixregions.html -- 7.3 Кб -- 01.10.2012
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13. SPUTNIK home page
... Average resolution at altitude H=668 km . ... Swath width at H=668 km and inclination of beginning of swath 20.48 degrees . ... Resolution at H=668 км . ... Наименование параметра . ... 1 канале . ... Полоса обзора при H=668 км . ... 1-5 спектральной зоне, не более . ... 1 спектральной зоне . 0,48-0,52 мкм . ... 0,915-0,997 мкм . ... 1-4 канал . ... 1-4 каналов . ... Спектральные характеристики каналов (по уровню 0,5): . ... For more information send a mail to: info@sputnik.infospace.ru . ...
[ Сохраненная копия ]  Ссылки http://sputnik.infospace.ru/ocean_o/engl/ocean_1.htm -- 19.8 Кб -- 21.01.2002
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15. Vladimir Marsakov Abstracts
... Using the uvby -photometry and proper motion data for about 5500 F stars within 80 pc from the Sun, we have studied velocity ellipsoid parameters and obtained the following results. 1) The sizw of all wllipsoid semiaxes increase systematically for groups of stars with the decrease of both temperature (at constant metallicity) and metallicity (at constant temperature). ... As a result, each of the three parameters - temperature, metallicity and velocity dispersion - is an age indicator. ...
[ Сохраненная копия ]  Ссылки http://ip.rsu.ru/~marsakov/abs/abst22.htm -- 5.4 Кб -- 02.02.2007
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16. sgs summary
... Guider functions . ... Guide Sensor Performance . ... Guide Sensor Sky Coverage/ Star Availability . Guide Star Selection Criteria . ... Guide fiber organization and reach at plug plate . ... Plug plate holes for guide stars are identical to those for science FO . ... FOV for each of 9 guide stars is 7.4 arcsec dia. (0.45 mm FO, Sumitomo IGN-05/10) . ... Selected guide stars must have no neighbor stars within TBD (5 arcsec) radius that have a brightness within TBD (5 mag.) of guide stars . ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/SDSS/eng.papers/19990324_guider/19990324.html -- 19.2 Кб -- 26.03.1999
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17. Specifications
... This function can also be used for particular types of subtypes or kinds: KIND (0) integer KIND (0.0) floating point number KIND (.FALSE.) logical variable KIND ("A") string of characters There is an intrinsic function SELECTED_REAL_KIND , which returns the kind of the type REAL that has a representation with (at least) the precision and the exponential range requested. ... With the choice SELECTED_INT_KIND (5) all integers between (but not including the limits) -100 000 and +100 000 are permitted. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/f77to90/c2.html -- 7.8 Кб -- 17.02.1996
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/f90/c2.html -- 7.8 Кб -- 17.02.1996
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18. 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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19. Biosphere: Analysis of Value Parameters
... Публикации и издания Публикации профессорско-преподавательского состава СГАУ Издания проф. Сосниной Т.Н. Biosphere: Analysis of Value Parameters . ... Besides, the ways of saving the use value and value properties of biosphere are analyzed. The expediency of transformation of two-criterion theory of value into the three- criterion theory of the balance of value, where the ecologic component performs the function of the key criterion has been founded. ... BIOSPHERE USE VALUE OF THE PRODUCT: MAIN . ...
[ Сохраненная копия ]  Ссылки http://www.ssau.ru/resources/sotrudniki/sosnina/mono14/ -- 80.9 Кб -- 10.04.2015
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20. http://selena.sai.msu.ru/Pug/Publications/ms42/m42_60.pdf
THE PARAMETERS INVOLVED IN HAPKE'S MODEL FOR ESTIMATION OF THE COMPOSITION OF THE EJECTA LUNAR TERRAINS. ... In the previous papers we were estimated the surface roughness of the ejecta lunar terrains by means comparison of the local phase function and the average integrated lunar indicatrix. ... The Hapke's theoretical model of the lunar surface reflection. ... For THE PARAMETERS INVOLVED IN HAPKE'S MODEL: S.G. Pugacheva, V.V. Shevchenko a low-albedo lunar surface parameter Bo = 1. ...
[ Текст ]  Ссылки http://selena.sai.msu.ru/Pug/Publications/ms42/m42_60.pdf -- 43.9 Кб -- 06.10.2008
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