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81. RAS ISR' Conclusion on the scientific results received in the orbital complex
... Director of the RAS ISR . RAS Academician . ... Astrophysics module Kvant of the orbital complex Mir launched in 1987 contains the largest on the station complex of the scientific equipment named the orbital observatory Roentgen. Observatory Roentgen consists of 4 X-ray telescopes, jointly exceeding the range of energies from 2 to 800 keV. ... Among the most significant results that were received in the observatory Roentgen are: . ... measurement of the periods of 9 X-ray pulsars; . ...
[ Сохраненная копия ]  Ссылки http://www.cosmoworld.ru/mirstation/english/documents/iki_ran_280998.shtml -- 11.0 Кб -- 09.04.2016
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82. Physicists from Samara and Novosibirsk discovered a new phenomenon
... Scientists from G. I. Budker Institute of Nuclear Physics- Syberian Branch of the Russian Academy of Science, Novosibirsk State University, Novosibirsk State Technical University, Samara State Aerospace University (SSAU) and Image Processing Systems Institute (IPSI) of the Russian Academy of Science, became the first people in the world obtained terahertz non-diffractive twisted Bessel beams and used them for the first time the formation of surface electromagnetic waves on the metal surface. ...
[ Сохраненная копия ]  Ссылки http://www.ssau.ru/engnews/11891/ -- 26.2 Кб -- 23.10.2015
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83. Full moon eclipse 9 november 2003
... Full silvery Moon illuminates terrain. ... Begun a next moon eclipse, when Land barriers a Moon from the Sun and throws its shade on it. ... Drawing 1. ... Drawing 6 Drawing 6 shows a splendid photo of full moon eclipse 18-19 november 1975 during is packed phases doing Dennis de Chikko. ... Eclipse, which will occur 9 november 2003, is a repetition through сарос (cycle of repetitions of eclipses equal 6585 days or 18 years 11 days) full moon eclipse from 28 octobers 1985 with the maximum phase 1,07....
[ Сохраненная копия ]  Ссылки http://www.moscowaleks.narod.ru/mooneclipse031109.html -- 18.5 Кб -- 09.04.2016
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84. Lunar Drawings
Crater Gassendi . ... I made this drawing was made on the 26th of november 2001. If you compare this one with the previous drawing of Gassendi (below) the differences are clear. ... This drawing was made on the 28th of september 2001. After nearly a full month without observations I had a one hour gap between the thicker clouds. ... This drawing was made on the 29th of august 2001. ... This drawing was made on the 27th of august 2001. ... This drawing was made on the 25th of august 2001. ...
[ Сохраненная копия ]  Ссылки http://aberrator.astronomy.net/moon/index.html -- 13.5 Кб -- 28.11.2001
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85. Proper motions of 59766 stars with respect to galaxies in 149 areas of the sky
The starting page - The catalogues page - The list of the PUL2 fields - The list of the Pul-3(Pul-3SE) fields - The list of the PUL_ERS fields . please read short description of the access form controls . ... Relative proper motion in RA *cos(DE), arcsec/yr . ... s. e. relative proper motion in RA *cos(DE), arcsec/yr . ... Number of Pul2 area . ... Check the apropriate checkbox to output these data and radiobutton to select stars within interval. back to the list of the Pul2 fields . ...
[ Сохраненная копия ]  Ссылки http://www.puldb.ru/pul2/pul2f.php?fn=001&ra=00%2009%2008.6&de=+27%2045%2047 -- 13.0 Кб -- 09.04.2016
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86. Uppsala General Catalogue of Galaxies
VII/26D Uppsala General Catalogue of Galaxies (UGC) (Nilson 1973) ================================================================================ Uppsala General Catalogue of Galaxies (UGC) Nilson P. =1973ugcg.book.. ... The order of the records is strictly by UGC number; i.e., the Addenda records follow their main catalogue counterparts in the file. ... Major axis of the galaxy as measured on the POSS blue print. ... References: Nilson, P. 1973, Uppsala General Catalogue of Galaxies, Uppsala Astron. ...
[ Сохраненная копия ]  Ссылки http://vega.inp.nsk.su/catalogs/ugc-description.php3 -- 15.1 Кб -- 01.10.2012
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87. 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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88. VaST homepage
... VaST is a software tool for finding variable objects on a series of astronomical images. ... VaST performs object detection and aperture photometry using SExtractor on each image, cross-matches lists of detected stars, performs magnitude calibration with respect to the first (reference) image and constructs a lightcurve for each object. ... VaST FITS image viewer ./pgfv . ... Part I" PZP, vol. ... K. V. Sokolovsky, S. A. Korotkiy; "New Variable Stars Discovered by the NMW Survey" PZP, vol. ...
[ Сохраненная копия ]  Ссылки http://scan.sai.msu.ru/vast/ -- 122.2 Кб -- 21.02.2016
[ Сохраненная копия ]  Ссылки http://saistud.sai.msu.ru/poisk/ -- 122.2 Кб -- 21.02.2016
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89. http://www.jsc.nasa.gov/roundup/online/2006/1206_p5_8.pdf
segments of the space station. ... Curbeam and Fuglesang will conduct the first spacewalk on Flight Day 4 to assist with the installation of P5 to P4. ... The mission's second spacewalk is set for Flight Day 6. ... NASA/Sowa STS116-S-002 Roundup 05 NASA STS121-S-030 STELLAR NEWS Hubble re-servicing mission a `go' S pace shuttle astronauts will make one final house call to NASA's Hubble Space Telescope as part of a mission to extend and improve the observatory's capabilities through 2013. ...
[ Текст ]  Ссылки http://www.jsc.nasa.gov/roundup/online/2006/1206_p5_8.pdf -- 2795.5 Кб -- 15.12.2006
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90. http://www.mccme.ru/dfc/2012/reports/Kaledin_report-2014.pdf
... More concretely, the sub ject of my research was a new homological invariant of associative algebras that I call "Hochschild-Witt homology a non-commutative generalization of de Rham-Witt complex of Deligne and Illusie. The realistic part of the pro ject was to define it for DG algebras, and then to prove that for a finite-dimensional algebra over a field, there is a comparison theorem that expresses pro-p completion of K-theory in terms of Hochschild-Witt homology. ...
[ Текст ]  Ссылки http://www.mccme.ru/dfc/2012/reports/Kaledin_report-2014.pdf -- 105.6 Кб -- 15.12.2014
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91. ICLP 2003, International Conference on Logic Programming, Mumbai (Bombay),...
. 5.24. Now I am in the Aeroflot plane. I discovered that I had become estranged from Russian people. The Russian personnel looks a bit strange for me.
[ Сохраненная копия ]  Ссылки http://www.cplire.ru/Lab144/iclp2003/5_24.html -- 1.6 Кб -- 24.09.2007
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92. rus
VIEW OUT OF THE WINDOW FROM FRANKFURT, GERMANY . ... Thank you very much for your very warm message (even though it is . very cold where you are!) ... other people see their world. ... our computer is into the garden in a small town called Griesheim, which is 33 kilometers south of Frankfurt. ... There is still a little snow on the grass and a couple of birds are hopping around and then suddenly one flys into our window. ... We are looking forward to Spring and much longer days when the birds . ...
[ Сохраненная копия ]  Ссылки http://edu.zelenogorsk.ru/eprojects/view/germany.htm -- 4.7 Кб -- 04.01.2001
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93. February 2002 APT Meeting
... APT Activities and Science Results 3. ... APT Secretary Philip Edwards (ISAS) reviewed the aims of the APT (http://www.vsop.isas.ac.jp/apt/DefinitionAndAims.html). ... The Australia Telescope Compact Array, and Ceduna, Hartebeesthoek, Kashima, Mopra, Parkes, and Shanghai telescopes of the Asia-Pacific Telescope participated in these observations. ... In the absence of Tetsuo Sasao, Philip Edwards briefly described results of the APT 22 GHz observations conducted from October 1st to 5th, 1997. ...
[ Сохраненная копия ]  Ссылки http://www.vsop.isas.ac.jp/apt/meetings/APTfeb2002summary.html -- 5.3 Кб -- 23.10.2002
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94. Keywords_312
Estimating the NEO Population and Impact Risk: Past, Present and Future . ... Since most of the risk resides in the largest impactors, finding that fraction of the largest bodies, and that none of them has a significant chance of impacting in the next century or so, "retires" more than 90 % of the impact risk, including most of the risk of a globally catastrophic impact event. ... In the mid-size range, from ~150 m to ~1 km, the main risk is from tsunami generated by an ocean impact. ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/EDITION/transaction/tbook/312.htm -- 6.9 Кб -- 02.10.2012
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95. SMIS IKI RAN (Equipmaent)
... Satellite data ] . ... The SCANOR system provides receiving and processing of the Earth-surface pictures made in visible and infra-red bands and transferred by satellites of the NOAA polar orbiter series (in the HRPT mode). ... The SCANOR system includes the desktop receiving device connected to an IBM AT 386 type computer, and the parabolic antenna with the guiding mechanism. The SCANOR system possesses the state-of-art software providing registration and processing of the received data. ...
[ Сохраненная копия ]  Ссылки http://smis.iki.rssi.ru/inform/engl/equip_e.htm -- 6.3 Кб -- 12.01.1999
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96. Star trails
... 16-mm/2.8 Fish-eye . ... I set up my Edixa Prismaflex TTL on a tripod outside the dome at Zeiss 50" and opened the camera for several hours. The 2.6 m Shain reflector is visible at center. The time exposure of about 5 hours duration showing circumpolar stars. The dome can be seen to blur slightly due to their motion during the exposure. Back to Astronomical Images Home Page . ...
[ Сохраненная копия ]  Ссылки http://www.vrum.chat.ru/Photo/Astro/StarTrak.htm -- 4.4 Кб -- 09.04.2016
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97. Celestia или как там ее - Астрософт
... Астрософт (Модератор: tlgleonid ) > . Celestia или как там ее . ... Right drag: orbit the selected object . ... Ctrl + Left drag: adjust distance to selection . Shift + Left drag: change field of view (e.g. => telescopic view) . Wheel (middle button) click: toggle field of view between 45 degrees . ... Chase selected object (orientation is based on selection's velocity) . T : Track selected object (keep selected object centered in view) . ... Ctrl+P : Mark selected object . ...
[ Сохраненная копия ]  Ссылки http://www.astroclub.kiev.ua/forum/index.php?topic=2051.0 -- 61.8 Кб -- 09.04.2016
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98. SAI Open Star Clusters (SAI OCL) Catalog
... Structure of Data . ... Catalog . ... In SAI OCL Catalog, we introduce our work on investigation of the Milky Way system of open star clusters. The main goal of our study is a search for new clusters using huge surveys. 168 new clusters have been already discovered by us using J,H,Ks data from 2MASS point source catalog. ... For 141 new clusters, we found their physical parameters using J,H,Ks data from 2MASS catalog and, for a number of clusters, our UBVRI CCD observational magnitudes. ...
[ Сохраненная копия ]  Ссылки http://ocl.sai.msu.ru/ -- 5.0 Кб -- 09.04.2016
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99. Спец.выпуск N5 (октябрь, 1999).
... Spacecraft that will search for planetary systems around 40 million stars and observe the largest explosions in the universe have been chosen as the next two missions in NASA's medium-class Explorer (MIDEX) program. ... The first mission, to be launched in 2003, is the Swift Gamma Ray Burst Explorer, a three-telescope space observatory for studying gamma ray bursts. ... During its three-year mission, Swift will also survey the sky for new black holes and other sources of cosmic gamma rays. ...
[ Сохраненная копия ]  Ссылки http://astrocourier.chat.ru/1999/99oct/99oct5.htm -- 15.5 Кб -- 09.04.2016
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100. The Sunspot Observer - Visual indices of solar activity
Statistics of sunspot activity . The sunspot indices . ... Visual indices of solar activity . ... n - number of spot groups . A - Waldmeier class of unipolar spot groups without penumbra . B - class of bipolar spot groups without penumbra . C - class of bipolar spot groups with one penumbra pole . D - class of small bipolar spot groups with two penumbra poles . E - class of middle bipolar spot groups with two penumbra poles . ... H - class of unipolar penumbrated spot groups . ...
[ Сохраненная копия ]  Ссылки http://www.alexeyryback.ru/en/sunspot_indices.htm -- 5.5 Кб -- 03.02.2016
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