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1. Dynamic HTML in Communicator
Contents] [Prev page] [Next page] [Index] . Navigator 4 from Netscape, which is part of the Communicator product suite, includes three new areas of functionality that taken together give you Dynamic HTML. The three components of Dynamic HTML are style sheets, content positioning, and downloadable fonts. Used together, these three components give you greater control over the appearance, layout, and behavior of your web pages. ... Introducing Downloadable Fonts . ...
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Ссылки http://crydee.sai.msu.ru/~vab/html.doc/dhtml/dynhtml/intro.htm -- 7.8 Кб -- 13.08.1997
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2. TUI:Telescope:Offset Types
TUI supports the following offsets: . Object Arc offset by a given amount on the sky (i.e. along the arc of a great circle). ... Arc offsets are useful for moving a different portion of your object or a different nearby object onto the boresight . ... Object Arc XY this is identical to an Object offset except that it has been rotated to align along the instrument x-y axes. ... This is just like the Calibration XY offset, except that it is typically cleared when you slew to a new object. ...
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Ссылки http://www.apo.nmsu.edu/35m_operations/TUI/Telescope/OffsetTypes.html -- 6.3 Кб -- 05.09.2014
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3. The AstroStat Slog Blog Archive [ArXiv] component separation methods
... Archives . ... The PCA and ICA is used for separating mixed components with some assumptions. ... The need of source separation methods in astronomy has led various adaptations of decomposition methods available. ... I rarely come up with a paper which gathered and summarized component separation methods applicable to astronomical data. In that regards, the following paper seems useful to overview methods of reducing dimensionality for astronomers. [arxiv:0805.0269] . ... Chandra Blog . ...
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Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2009/arxiv-component-separation-methods/index.html -- 23.2 Кб -- 01.03.2014
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4. casacore: components/ComponentModels/ComponentType.h Source File
... Classes . Files . ... Astronomy Observatory 00023 //# 520 Edgemont Road 00024 //# Charlottesville, VA 22903-2475 USA 00025 //# 00026 //# 00027 //# $Id: ComponentType.h 20299 2008-04-03 05:56:44Z gervandiepen $ 00028 00029 #ifndef COMPONENTS _COMPONENTTYPE_H 00030 #define COMPONENTS _COMPONENTTYPE_H 00031 00032 #include casa/aips.h 00033 namespace casac { 00034 class componentlist; 00035 }; 00036 namespace casa { //# NAMESPACE CASA - BEGIN 00037 00038 class String ; 00039 ...
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Ссылки http://www.atnf.csiro.au/computing/software/casacore/casacore-1.2.0/doc/html/ComponentType_8h_source.html -- 27.6 Кб -- 14.02.2011
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5. Magnetic fields, subatomic particles, etc., traveling in different directions
... Magnetic fields, subatomic particles, etc., traveling in different directions fill the universe. Do they deflect or otherwise affect one another? If so, isnт??t the information we get from them distorted? ... Neutrino astronomy, which is still in its infancy, is attractive because neutrinos interact so weakly with matter that few of these distorting effects occur. Get instant access to subscriber content on Astronomy.com! ...
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Ссылки http://www.astronomy.com/magazine/ask-astro/2011/03/when-particles-collide -- 63.4 Кб -- 10.04.2016
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6. APOD: 2000 January 4 - Galaxies Cluster Toward the Great Attractor
... 2000 January 4 . Galaxies Cluster Toward the Great Attractor . ... The galaxies pictured above are part of a cluster of galaxies called ACO 3627 near the center of the Great Attractor . ... The Great Attractor is a diffuse mass concentration fully 250 million light-years away, but so large it pulls our own Milky Way Galaxy and millions of others galaxies towards it. Many of the galaxies in ACO 3627 are slowly heading towards collisions with each other. ... About APOD > . ...
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Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/gacluster_wfi_big.html -- 4.7 Кб -- 04.03.2001
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7. Астронет > Jupiter: The Great Yellow Spot
... Jupiter: The Great Yellow Spot . ... Credit: The Galileo Project , JPL , NASA Explanation: What happened to Jupiter's Great Red Spot ? Operating at a chilly 55 degrees Kelvin , the Galileo Spacecraft's Near Infrared Mapping Spectrometer (NIMS) recorded this composite image of Jupiter's Great Red Spot in late June 1996. ... 1995 1996 1997 1998 . ... NASA Official: Jay Norris. ... Публикации с ключевыми словами: Jupiter - Большое Красное Пятно - ураган - инфракрасное излучение - Юпитер . ...
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Ссылки http://www.astronet.ru/db/msg/1163221/eng/ -- 22.3 Кб -- 22.06.2003
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8. Getting Started in Actor Prolog. Component-Oriented Programming.
The idea of component-oriented programming is that in the course of implementation of various software projects a programmer (or a programmers team) accumulates a library of reused software fragments that are used in different projects. ... To solve such problems there are some special syntax means in Actor Prolog that support component-oriented programming. ... A package in Actor Prolog is a set of classes linked by implication. ... Actor Prolog supports visual component-oriented programming. ...
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Ссылки http://www.cplire.ru/Lab144/start/e_comp.html -- 18.6 Кб -- 24.09.2007
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9. http://www.mccme.ru/dfc/2010/reports/2013-Kuyumzhiyan_Report.pdf
GROUPS OF ALGEBRAIC TRANSFORMATIONS OF AFFINE VARIETIES FINAL REPORT FOR THE THREE YEARS KARINE KUYUMZHIYAN 1. ... The latter is an algebraic variety with the given field of rational functions and an infinitely transitive regular action of a group of algebraic automorphisms generated by unipotent algebraic subgroups. ... Quotient groups. ... Since over R there exist irreducible non-connected varieties, we cannot have even one-transitivity of any connected group of automorphisms. ...
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Ссылки http://www.mccme.ru/dfc/2010/reports/2013-Kuyumzhiyan_Report.pdf -- 46.0 Кб -- 15.12.2013
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10. http://www.iki.rssi.ru/galeev/astro2007/krivosheyev2007.pdf
... Mass ratio of SS433 components is q = M X / MV = 0.2 В 0.3 . ... The spectum corresponds to precessional moment T3, i.e. when the angle between jet axis and the line of sight is equal 60 degrees. 10 -2 10 -3 lg I, phot/cm2/sec/keV 10 -4 10 -5 10 100 lg h, keV Cherepashchuk A.M.,Sunyaev R.A., Fabrika S.N., Postnov K.A. et al./ ... 5 10 100 Tcor = 20keV lg h, keV Mjet = 21020 g / s Lk = 61039 erg / s Angle dependence of SS433 spectrum In the figure the angle dependence for SS433 spectrum is shown. ...
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Ссылки http://www.iki.rssi.ru/galeev/astro2007/krivosheyev2007.pdf -- 389.1 Кб -- 27.02.2008
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11. http://www.iki.rssi.ru/seminar/20100609_11/Krivosheyev.pdf
... Moscow, Russia E-mail: krivosheev@iki.rssi.ru Notes: · · The Monte Carlo method (s) is also called the statistical test method An innumerable number of processes can be listed the outcome of which is not determined and has probabilistic nature, but these processes obey statistical laws, so to obtain the result we have to make multiple similar tests, i.e. to use the MC method Because probabilistic processes are widely spread in nature, the MC ...
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Ссылки http://www.iki.rssi.ru/seminar/20100609_11/Krivosheyev.pdf -- 663.0 Кб -- 29.06.2010
[ Текст ] Ссылки http://www.cosmos.ru/seminar/20100609_11/Krivosheyev.pdf -- 663.0 Кб -- 29.06.2010
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[ Текст ] Ссылки http://www.cosmos.ru/seminar/20100609_11/Krivosheyev.pdf -- 663.0 Кб -- 29.06.2010
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12. ASP: An Ancient Universe - Changes in Stars
An Ancient Universe: How Astronomers Know the Vast Scale of Cosmic Time . THE CHANGING UNIVERSE: EVOLUTION HAPPENS! . b) Changes in Stars . One of the great discoveries of modern science is that stars (like people) live only a measurable life-time and then die. Although the lives of the stars are enormously longer than the span of a human life, we can learn about the life story of the stars by studying them at many different stages in their life cycle, from birth to death. ...
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Ссылки http://www.astrosociety.org/edu/publications/tnl/56/changing2.html -- 10.5 Кб -- 02.10.2012
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13. Other interesting links
.
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Ссылки http://comet.sai.msu.ru/~dmbiz/Lrest.html -- 5.0 Кб -- 11.10.2004
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14. Second Cross-Border Science Conference "Great Success" | International Year of
... Armagh Observatory, 5th May 2009: The Second Cross-Border Schools Science Conference тАЬDiscover the Stars at ArmaghтАЭ, held on 29th and 30th April 2009 and organized by the Armagh Observatory and the Centre for Cross Border Studies was a great success. ... The conference was held as part of the ObservatoryтАЩs contributions to the United Nations International Year of Astronomy IYA2009. ... The first cross-border schoolsтАЩ science conference was held in Armagh in March 2007. ...
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Ссылки http://star.arm.ac.uk/scholars/iya/official_press_releases/ssc2009_great_success.html -- 9.9 Кб -- 31.12.2009
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15. (Untitled)
To proceed to drawing tracks of some objects select Tracks item in menu bar and then select Input Data in drop-down menu. Enter initial and final dates of time interval in corresponding data fields of the Input Data dialog box Input Data . ... The frame with horizontal and vertical scales corresponding to the right ascension and declination axes appears on screen. ... Depending on specifications introduced in the Input Data dialog box the picture represents tracks up to three different objects. ...
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Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user2pnr.htm -- 3.1 Кб -- 10.04.2016
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16. ADASS 2002 Conference Proceedings
... Fasti is a controller architecture originally developed for fast infrared astronomical array detectors, and intended to be powerful and extendible. ... 2002), Foppiani et al. 2002)). ... The parallel input interface (now a commercial board). ... Esposito, S., Riccardi, A., Storm, J., Accardo, M., Baffa, C., Biliotti, V., Foppiani, I., Puglisi, A., Ragazzoni, R., Ranfagni, P., Stefanini, P., Salinari, P., Seifert, W., Storm, J. 2002, SPIE Conference AS06, Wizinowich, P. L. Ed., in press . ...
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Ссылки http://www.adass.org/adass/proceedings/adass02/P8-5/ -- 12.0 Кб -- 13.03.2003
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17. Data Format Session at 2001 IAU WG Meeting
The preliminary version of documentation of the format for the interchange of calibrated optical/IR data being developed by Tom Pauls of NRL and John Young of COAST was presented and a number of issues discussed. The proposed format is in the general form of a relational database with different components stored in FITS binary tables. ... Should there be a single data table type that includes all data types, or multiple table types, one per data type? What data types are needed? ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/oi_data/cotton_report.html -- 5.8 Кб -- 11.01.2008
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18. Measurement of the dark halo shape in polar ring galaxies
... According to the most popular cosmological paradigm, the greater part of the galaxy mass is accumulated in the dark matter halo. ... The polar ring galaxies (PRGs) reveal external rings or disks of gas, dust and stars rotating in a plane roughly perpendicular to the disk of the central galaxy. ... The shape of the dark halo in the model was chosen so as to achieve the best fit to the observed rotation of both galaxies themselves and their polar rings. ... The SPRC-7 galaxy. ...
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Ссылки http://www.sao.ru/Doc-en/SciNews/2014/DMhalo/ -- 8.9 Кб -- 10.04.2016
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19. Carnival of Space No 178: a galaxy of space blogs | Astronotes
Astronotes Armagh Planetarium's Stellar Blog! ... Armagh Planetarium . ... Our Galaxy . ... Other Galaxies . ... Space Flight . ... This week?s€а Carnival is hosted by the excellent We Are All in the Gutter (Looking at the Stars) blog .€а You can go straight to the Carnival by clicking here. ... Hello, IтАЩm Colin, welcoming you to Astronotes, the PlanetariumтАЩs official blog. Here you will find the latest news and views from the fascinating worlds of astronomy and space exploration. ...
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Ссылки http://www.armaghplanet.com/blog/carnival-of-space-no-178-a-galaxy-of-space-blogs.html -- 40.3 Кб -- 09.04.2016
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20. Extinction properties (transmitted radiation)
Next: Extinction efficiencies: general behaviour Up: Optical properties of cosmic Previous: Optical properties of cosmic . It is now evident that observed interstellar extinction cannot be explain using particles of only one kind. ... The intensity of radiation after passing a dust cloud is equal to . ... The interstellar extinction is . ... Next: Extinction efficiencies: general behaviour Up: Optical properties of cosmic Previous: Optical properties of cosmic root 2003-04-09 ...
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Ссылки http://www.astro.spbu.ru/DOP/8-GLIB/ASTNOTES/node1.html -- 11.6 Кб -- 19.11.2010
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Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
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