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1. *ltcurv* - Generation of the light curve
Next: *ltcplot* - Plot the Up: Counting rate vs. time Previous: Counting rate vs. time . Produce a light curve for the source at 6940 9390, using timesorted QPOE file . input file: rp90_sti.qp . ... xt> ltcurv # In the timing package Input Source Timing File: rp90 # Only the root name is needed, # the default extension is known Input Background Timing File (NONE): <cr> # No bkg data rootname for output file: rp90 or . will assign same root name Number of Bins: 500 # 500 data bins xt> . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node171.html -- 3.9 Кб -- 01.10.2012
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2. Stellarium: StelGeometryBuilder Class Reference
Stellarium 0.12.3 . ... StelGeometryBuilder Class Reference . ... buildCircle ( StelVertexBuffer < VertexP2 > *vertexBuffer, const float x, const float y, const float radius, const int segments=128) . ... buildCylinder ( StelVertexBuffer < VertexP3T2 > *const vertexBuffer, const float radius, const float height, const int slices, const bool orientInside=false) . ... Build a fisheye-textured sphere. ... Build a flat texture mapped ring with 3D coordinates (for example for planet's rings) More.. ...
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/classStelGeometryBuilder.html -- 28.2 Кб -- 28.02.2014
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3. The Complex Ion Tail of Comet Lovejoy
... The Complex Ion Tail of Comet Lovejoy . ... As the name implies, the ion tail is made of ionized gas -- gas energized by ultraviolet light from the Sun and pushed outward by the solar wind. ... The effect of the variable solar wind combined with different gas jets venting from the comet's nucleus accounts for the tail's complex structure. ... NASA Web Site Statements, Warnings, and Disclaimers . ... Publications with keywords: comet - comet tail . Publications with words: comet - comet tail . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/1330916 -- 16.2 Кб -- 21.01.2015
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4. Худи Nike - Nike - Nike Шапка-бини детская Hemlig. 528425 528425-4830
... Цвет: черный . ... Худи Nike. ... Стильная теплая детская шапка Reima Hemlig идеально подойдет для прогулок в холодное время года. ... В комплект вошли монеты: 1. 10 драмов Диаметр 2,7 см. 2. 5 драмов Диаметр 2,5 см. 3. 3 драма Диаметр 2,3 см. 4. 1 драм Диаметр 2 см. 5. 50 лумов Диаметр 1,9 см. 6. 20 лумов Диаметр 1,6 см. 7. 10 лумов Диаметр 1,5 см. ... Цвет: розовый . ... Возраст: Детский . ... Диаметр, мм: 100 . Цвет плафонов и подвесок: алюминий, неокрашенный . Цвет арматуры: хром . ...
[ Сохраненная копия ]  Ссылки http://astrokuban.info/astroku4834.html -- 20.5 Кб -- 14.02.2016
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5. Radioastrophysical Observatory ISTP RAS SB
RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . Principle of generation of radio images General information Main characteristics of the Radio telescope Observing programs General view of the antenna array Main research areas Radio telescope's beam Receiving systems Main characteristics of the base receiving-recording complex Calibrations Data archive and databases ... Solar radio images are generated by beams oriented within the SSRT field of view (90'). ...
[ Сохраненная копия ]  Ссылки http://ssrt.iszf.irk.ru/rad15en.shtml -- 15.1 Кб -- 27.02.2014
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6. ESO reveals end of cosmic Dark ages | Astronotes
Astronotes Armagh Planetarium's Stellar Blog! ... Our Galaxy . ... Stars . ... Space Flight . ... New observations with the European Southern Observatory (ESO)тАЩs Very Large Telescope of some of the most distant galaxies ever detected are revealing the mysteries of this important phase of the early Universe. ... These powerful instruments are essential for exploring this early period in cosmic history as they alone can enable the accurate observations of €аthese extremely distant and faint galaxies. ...
[ Сохраненная копия ]  Ссылки http://www.armaghplanet.com/blog/light-from-the-end-of-the-dark-ages.html -- 46.5 Кб -- 09.04.2016
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7. Synthetic Images of the Solar Corona from Octree Representation of 3-D Electron
... Empirical and theoretical modeling of 3-D structures in the solar corona is confronted by the tremendous amount of data needed to represent phenomena with a large dynamic range both in size and magnitude, and with a rapid temporal evolution. Octree representation of the 3-D coronal electron distribution offers the right compromise between resolution and size, allowing computation of synthetic images of the solar corona. ... The time interval between images is one day. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass96/llebariaa2.html -- 12.0 Кб -- 23.06.1998
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8. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/Carina.txt
... STScI-PRC00-06 LIGHT AND SHADOW IN THE CARINA NEBULA Previously unseen details of a mysterious, complex structure within the Carina Nebula (NGC 3372) are revealed by this image of the "Keyhole Nebula," obtained with NASA's Hubble Space Telescope. ... This region, about 8000 light-years from Earth, is located adjacent to the famous explosive variable star Eta Carinae, which lies just outside the field of view toward the upper right. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/Carina.txt -- 4.8 Кб -- 30.01.2001
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9. Vitaly Goranskij, SAI/Moscow Univ.
... SCIENCE AND BUSINESS . Such a trifle as a starry night sky of largest observatories turned out to be a small change coin in commercial bargains for exclusive communal services in Russia, and for a few elite flats in penthouses in Ukraine. SCIENCE AND BUREAUCRATISM . ... Till in Russian) . ... Clericalization of science and education (Till in Russian). ... Researcher of the Sternberg Astronomical Institute, The Moscow University. ... SAI home page . ... October, 2008) . ... November, 2007) . ...
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/jet/~goray/ -- 6.7 Кб -- 07.08.2010
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10. Detection of polarized radiation sources with unusual spectral characteristics
... Solar flare activity is produced by the processes of accumulation and release of energy in an active region. ... In the framework of study of solar active regions, producing powerful flares the researchers from the RATAN-600 radio telescope have detected sources with features in the form of a sharp drop in the intensity of polarized radiation in various parts of the recorded frequency range (2-16GHz), sometimes changing the sign of polarization. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/SciNews/2011/Bogod/ -- 4.0 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/Doc-en/SciNews/2011/Bogod/ -- 4.0 Кб -- 02.10.2012
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11. Image: On the Observatory park alleys. Note the shielded street light
. Album : asv-album :: Travels to distant places and countries :: 1998/06 Nauchny, Katsively (Crimea, Ukraine) :: В Научном . Up . On the Observatory park alleys. Note the shielded street light (astronomers do not want extra light in the night) . Next >> . Photo album generated by album from D. Madison 's Marginal Hacks on Tue Jun 23 14:46:46 2015 .
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/album/trips/1998.06.Crimea/1.Nauchny/tn/d02l.jpg.index.html -- 6.1 Кб -- 23.06.2015
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12. Coupled dipoles method (Purcell-Pennypacker, CDM)
... In the western literature this method is now called ``coupled dipole method" (CDM). ... Thus, a system of equations relative to the fields scattered by the elementary domains can be obtained, and summation of these fields gives the total scattering field. ... A subtle difference between both methods is in the fact that in the first method one works with the fields which excite a dipole (without the field of the dipole), whereas in the second method one uses the real fields in a given domain. ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/DOP/3-REVS/KHLEB1/node9.html -- 10.2 Кб -- 19.11.2010
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13. http://scan.sai.msu.ru/lk/
Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...
[ Сохраненная копия ]  Ссылки http://scan.sai.msu.ru/lk/ -- 6.6 Кб -- 24.12.2015
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14. Studying the complex aftermath of a supernova | Astronomy.com
... Tonight's Sky . ... Star Atlas . ... Supernova showered Earth with radioactive debris . ... stars . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Astronomy for Kids . ... Studying the complex aftermath of a supernova . ... An asymmetric supernova explosion may have given a recoil kick to the pulsar, causing it to move rapidly and drag the pulsar wind nebula along with it. ... Only registered members of Astronomy.com are allowed to comment on this article. ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/news/2014/11/studying-the-complex-aftermath-of-a-supernova -- 69.4 Кб -- 10.04.2016
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15. Taurid Complex
Orbital intersection . ... Structure of Taurid stream . ... Meteoroid swarm and Taurid fireballs . ... The following four diagrams schematically show four different Taurid orbits and the orbits of Earth and Jupiter. ... The Taurid stream contains particles (small, solid grains) at different stages of their precession cycles. ... The study of when a meteor stream can produce a meteor shower is the study of when precession brings orbits to intersection with Earth, or e.g. with Mars . ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~aac/zetataur.html -- 8.7 Кб -- 19.10.2007
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16. astro-ph
... arXiv.org . ... Modeling Light Curves for Improved Classification . ... These include heterogeneity of the data, irregularly sampled data, missing data, censored data, known but variable measurement errors, and most importantly, the need to classify in astronomical objects in real time using these imperfect light curves. We describe a modeling-based approach using Gaussian process regression for generating critical measures representing features for the classification of such lightcurves. ...
[ Сохраненная копия ]  Ссылки http://vo.astronet.ru/arxiv/?get_articles=1&author=Yi -- 8.0 Кб -- 13.04.2016
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17. A computer controlled low light photometer for nightglow observations
A computer controlled low light photometer for nightglow observations. Hardware units of portable photometer for low light measurements, especially night glow emission is described. ... Interface card contain three channels of 24 bit counter, 4 channels of 12 bit ADC and the buffer bus for the controlled motors of the altazimuthal fork mounting and filters wheel, the position encoders. ... Where N( ) is output signal photometer generated input light flux F( l ) . ... PMT # . 599 . ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/~lapchuk/Photometer.htm -- 15.9 Кб -- 21.02.2000
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18. Complex evaluator
CALCSYM - complex evaluator . ... CALCSYM.exe and CALCSYMi.exe will allow you to obtain numeric solution for *.out file generated by both CIRSYM and MATSYM programs (computation of freqency responces, unknowns, determinants, sensitivity analysis etc.. ... Setup file name for CALCSYM is "setup.cal". ... CALCSYMi.exe will allow you to work with long double over the range from 3.4*E-4932 to 3.4*E+4932. ... To calculate, run CALCSYM.exe and enter "file_name.OUT" or click on the "ENTER" (in "OUT" case). ...
[ Сохраненная копия ]  Ссылки http://astrometric.sai.msu.ru/~symbol/calcsym.html -- 2.6 Кб -- 06.10.2004
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19. Light baffle installation
... The light baffles consist of the wind baffle that surrounds the telescope and doubles as a light baffle, the primary baffle that extends from the primary center-hole toward the secondary (left), the secondary baffle that extends from the perimeter of the secondary toward the primary (right), and the conical baffle that is suspended approximately halfway between the primary and secondary (middle). The wind baffle is covered with panels that are 25% porous to the wind. ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Site/SDSS.progress/19980524_Baffle_Installation/19980524.html -- 6.9 Кб -- 28.05.1998
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20. RTT150 Technical Description
RTT150 . ... The primary mirror 1 reflects light to the secondary mirror 2 which collects it on the focal surface of system with the linear field of 30 mm diameter. Focal length, mm . ... Linear field of view, mm . ... Angular field of view . ... Concentration of light energy at 632.8 nm wavelength . on the optical axis within the circles of diameter: . 0.036 mm, %, at least . ... 0.060 mm, %, at least . ...
[ Сохраненная копия ]  Ссылки http://hea.iki.rssi.ru/AZT22/ENG/to_f1160.htm -- 4.5 Кб -- 18.02.2004
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