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http://xmm.vilspa.esa.es/sas/6.5.0/doc/esensitivity/node5.html.
http://xmm.vilspa.esa.es/sas/6.5.0/doc/esensitivity/node5.html.
21. Tatjana Khruzina
... For the past years I have been working on the problem of synthesis of light curves of close binary systems, consisting of a normal star and a compact object (point object with fixed X-ray luminosity). ... Possible existence of a bright spot on the disk's lateral surface is taken into account. ... The last of then will be published in Gordon and Breach Publishers ( Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ... Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ...
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Ссылки http://uranus.sai.msu.ru/~kts/ -- 4.4 Кб -- 22.09.2000
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22. 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. ...
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Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/impol/polimodel.help.html -- 6.1 Кб -- 06.06.2006
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23. 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. ...
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Ссылки http://www.eso.org/~jwalsh/softpol/polimodel.help.html -- 6.1 Кб -- 02.11.2000
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24. Pulkovo Astrometrical Plate Database
Pulkovo Photographic Plate Database . To find a certain plate, type its number, choose instrument and click button FIND Instrument: Normal Astrograph 26-inch refractor Plate number: . To find plates with a certain sky area: choose instrument, type coordinates (R.A. and Dec.) of the center of this area, type radius of this area, type (optionally) names of required objects, and click button FIND . ...
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Ссылки http://www.puldb.ru/db/plates/index.php -- 6.7 Кб -- 01.10.2012
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25. Pictures/Рисунки
This is how a typical dispersion modeling result looks when shown as a map. ... Their numerical values are shown at the top. White normally means no data, but high values may be also shown as white if above the fixed high limit (that is, if no automatic normalization is used for colors). Note that calculations were done both for cell positions and for station positions, so both are colored. PO territories are filled by color corresponding to the average value of cells overlaying them. ...
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Ссылки http://www.iki.rssi.ru/ehips/Australia/NCF2.htm -- 2.3 Кб -- 20.09.2001
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26. Untitled Normal Page
. Visitors of my Home Page: . љ . Back to Home Page . Personal information . Alexander Konovalenko alex.kono@mailcity.com
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Ссылки http://space.univ.kiev.ua/~kono/last.html -- 2.2 Кб -- 15.02.2000
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27. Description of the RadioAstron project, english version
Orbit . ... The orbit of the RadioAstron provides four types of study: . rough images of radio sources with ultra-high angular resolution, using all baselines up to the radius of the apogee, that is much larger than Earth diameter; . ... high quality imaging of radio sources, with moderate resolution, by observing either with small projected base lines Earth-spacecraft, i.e. close to the orbital plane, or near the perigee. ... high accuracy orbit determination. ... Space Radio Telescope . ...
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Ссылки http://www.asc.rssi.ru/RadioAstron/description/orbit_eng.htm -- 7.3 Кб -- 10.05.2008
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28. Keywords_152
Electronic Catalogue of Comets "Halley" . ... In this paper we give a description of the Electronic Catalogue of Comets "Halley", which makes it possible to calculate the evolution of the orbits of comets, to visualize orbital motion, to determine the circumstances of a comet's close approach to planets within a given time interval, as well as a number of other opportunities. ...
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Ссылки http://www.ipa.nw.ru/PAGE/EDITION/transaction/tbook/152.htm -- 4.3 Кб -- 02.10.2012
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29. Description of SED models
... FTP access the basic models is here . ... Below, we put short descriptions of the used SED models for the photometric redshifts providing by the current server . ... The uniqueness of this model consists in expanding to the near IR (NIR) of Rocca-Volmerange and Guiderdoni's (1988) atlas of synthetic spectra with a revised stellar library, which includes parameters of cool stars. ... Homepage of the GISSEL model). ... Another model used earlier is the model of synthetic spectra of Poggianti (1997). ...
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Ссылки http://sed.sao.ru/sed_E_models.html -- 9.2 Кб -- 12.01.2005
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30. Summary of Friction
.
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Ссылки http://zebu.uoregon.edu/1995/ph161/friction.html -- 4.9 Кб -- 23.09.1997
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31. SAI OCL Catalog Description
... Description . Catalog . ... In the Catalog, we publish equatorial (ЮБ 2000 , ЮД 2000 ) and galactic (l,b) coordinates of cluster centers derived as the position of overdensity in 2MASS catalog (Koposov et al. ... Distances, color-excesses and ages are the mean-square values calculated using all available evaluations from different color-magnitude diagrams. ... There are individual pages for every cluster where all available plots and parameters are published. ... 2002). ...
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Ссылки http://ocl.sai.msu.ru/description/ -- 5.9 Кб -- 09.04.2016
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32. If neutron stars don't produce energy from fusion, like normal stars, how can
... Star Atlas . ... stars . ... If neutron stars don't produce energy from fusion, like normal stars, how can they shine in visible light? ... Although it is true that neutron stars have, for the most part, consumed all their internal thermonuclear fuel, they tap into other energy sources to produce light. Indeed, neutron stars are remarkably "resourceful" and employ a variety of physical mechanisms to make themselves visible.A newborn neutron star is incredibly hot ? ... Atlas of the Stars . ...
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Ссылки http://www.astronomy.com/magazine/ask-astro/2005/03/if-neutron-stars-dont-produce-energy-from-fusion-like-normal-stars-how-can-they-shine-in-visible-light -- 63.4 Кб -- 10.04.2016
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33. ASCII files description
... Co-ordinate systems description . Directories structure . The file names' construction . The file set description . ... The orbital information for each month is presented in the separate directory. The INTERBALL orbital data are located on the STDA server, for each month in the separate subdirectory, which name consists from the year (YYYY) and month (MM) numbers. The Parent Directory of the Tail Probe orbital data is http://www.iki.rssi.ru/da/interball/tail/orbit/ . ...
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Ссылки http://www.iki.rssi.ru/vprokhor/camp2/numfile.htm -- 9.9 Кб -- 06.06.1999
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/vprokhor/camp2/numfile.htm -- 9.9 Кб -- 06.06.1999
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[ Сохраненная копия ] Ссылки http://www.cosmos.ru/vprokhor/camp2/numfile.htm -- 9.9 Кб -- 06.06.1999
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34. A Computer-Based Technique for Automatic Description and Classification of
... A technique allowing automatic representation by a relatively small number of independent parameters based on the principal component analysis of data sequences is presented. ... In recent years the spectrum of observed astronomical data can be characterized as greatly varied. ... In this instance, the problem of initial description and classification of newly-observed data becomes most urgent, especially if there is a lack of preliminary observational material and theoretical expectations. ...
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Ссылки http://www.adass.org/adass/proceedings/adass96/vasilyevs.html -- 11.6 Кб -- 23.06.1998
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35. XV-MULTI
. Russian Version [ MS-Win ] . [ News ] . [ Satellite data ] . [ SMIS ] . [ ] . The program processes multi-band images to detect homogeneous areas and perform image classification. It includes a number of segmentation algorithms. The classification can be performed using various methods - nearest neighbor, normalized distance, estimate calculation. Demo version . Price . Back to SMIS Home Page .
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Ссылки http://smis.iki.rssi.ru/inform/engl/soft/e_multi.htm -- 3.2 Кб -- 13.03.1997
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36. SIXA acceptance tests, 2000
... SIXA FM ACCEPTANCE TESTS . ... In accordance to plan of the Acceptance Tests for Flight Models which was agreed in March 2000 in Moscow, the Acceptance Test of SIXA FM was carried out between 28 August and 2 September at VTT Automation, Finland. ... GOUCH for electronics box of SIXA-FM, Remark: not updated after changes made in 1994. ... Ground Test Program of SIXA-FM. ... Integration Test of SIXA FM, BIUS, ISS, DSS, and MPMI . ... Test data were written to MPMI, DSS-F, DSS-S and GSE SIXA-FM, . ...
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Ссылки http://hea.iki.rssi.ru/SXG/sixa/acc2000.htm -- 11.5 Кб -- 18.02.2004
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37. http://www.gao.spb.ru/english/as/j2014/presentations/huang.pdf
Do we need various assumptions to get a good FCN? A new multiple layer spectral method Cheng-li HuangMian Zhang Shanghai Astron. ... No FCN ! ... FCN,FCN,FCN.. Multiple layer spectral method (MLSM) + Linear Operator Method (LOM) Finite Element Method (FEM) · · Traditional approach solves one order ellipsoid only. ... Main Idea of FEM Boundary Surface could be described as: Let's consider how to solve the dynamic equation: Traditional Approach: Equivalent Spherical Domain . ...
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Ссылки http://www.gao.spb.ru/english/as/j2014/presentations/huang.pdf -- 1455.6 Кб -- 28.09.2014
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38. Vladimir Marsakov Abstracts
... The normal m 1 , c 1 indices and metallicities have been calculated for 2472 F-stars from the uvby and H fotometry. ... It is shown that the metallicity distribution of F6-G0 dwarfs is not a Gaussian one, but may be considered as a sum of two normal distributions. At the centre, the distribution shows a gap which subdivides all the stars into two metallicity groups. ... По данным uvby , H - фотометрии вычислены нормальные индексы m 1 , c 1 и определена металличность 2472 F-зыезд. ...
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Ссылки http://ip.rsu.ru/~marsakov/abs/abst10.htm -- 3.7 Кб -- 02.02.2007
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39. http://www.cplire.ru/html/lab234/pubs/2005-18.pdf
On the concept of a cold-electron bolometer mixer M. Tarasov1,2, and L. Kuzmin1 Chalmers University of Technology, KemivДgen 9, SE-41296 GЖteborg, Sweden Institute of Radio Engineering and Electronics, Mokhovaya 11 bld. ... CEB mixer combines advantages of Hot Electron Bolometer (HEB) mixer such as high signal frequency and low LO power, and advantages of SIS mixer such as low noise, high IF and immunity to small temperature variations. ... Finally for CEBM we can have moderate power gain. ...
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Ссылки http://www.cplire.ru/html/lab234/pubs/2005-18.pdf -- 24.3 Кб -- 24.01.2006
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40. http://www.apo.nmsu.edu/Site/030107FacTrbleShoot/GeneratorTransferSwitch.pdf
GENERATOR TRANSFER SWITCH Page 1 of 9 Power Distribution: Normal Operating Conditions All site power comes into panel MDP on the loading dock. ... Figure 1 GENERATOR TRANSFER SWITCH Page 3 of 9 Under normal conditions, the transfer switch routes power from panel MDP to all loads in panels DPE (near Washer/Dryer) and SDP (in boiler room). ... GENERATOR TRANSFER SWITCH Page 5 of 9 Figure 3 Method #3 This method requires manual activation of the Generator and transfer switch. ... Generator should start. ...
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Ссылки http://www.apo.nmsu.edu/Site/030107FacTrbleShoot/GeneratorTransferSwitch.pdf -- 298.9 Кб -- 18.07.2014
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