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41. Research Laboratory of the "Analytical instruments and systems' (RL-54)
... Events . ... Pre-university education . ... Research areas . ... Samara region . ... Samara State Aerospace University Research Research and education centers Research Laboratory of the "Analytical instruments and systems' (RL-54) . ... Development of control systems by applying a protective coating on the inner surface of pipes. Development of non-contact optical and acoustic systems for measurements of geometric parameters of profile products , including pipeline facilities. ...
[ Сохраненная копия ]  Ссылки http://www.ssau.ru/english/research/research_n_education/rl_54/ -- 23.6 Кб -- 10.04.2015
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42. To gravitational wave discovery with LIGO
The direct detection of gravitational waves is one of those events long-expected by physicists that are nevertheless a significant occurrence which excites the world scientific community as if something unexpected has happened. ... Many rumors leaked ahead of the conference, and the fact that something (that is, a signal corresponding to gravitational waves) was discovered by LIGO (Laser Interferometer Gravitational-Wave Observatory) was discussed on the sidelines. ... arXiv:1602.03868 . ...
[ Сохраненная копия ]  Ссылки http://sed.sao.ru/~vo/LIGO/gravw_en.html -- 46.9 Кб -- 21.03.2016
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43. APOD: October 17, 1999 - Black Holes in Galactic Centers
... October 17, 1999 . Black Holes in Galactic Centers . ... HST , NASA . Explanation: Do all galaxies have black holes at their centers? Although not even a single galaxy has yet been proven to have a central black hole , the list of candidates continues to increase. ... In all the galaxies studied, star speeds continue to increase closer the very center . This in itself indicates a center millions of times more massive than our Sun is needed to contain the stars. ... About APOD > . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap991017.html -- 4.5 Кб -- 02.10.2012
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44. ASP: A Taste of Real Astronomy ? The ESA/ESO Astronomy Exercises
The ESA/ESO Astronomy Exercise Series 2 . The Distance to Messier 100 as Determined by Cepheid Variable Stars . ... The small variations in distance to the individual Cepheid variable stars in the Cloud are negligible compared with the much larger distance to the SMC. ... In this way Cepheid variable stars can be used as one of the 'standard candles' in the Universe that act either as distance indicators themselves or can be used to calibrate (or set the zero point for) other distance indicators. ...
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/edu/publications/tnl/57/realastro3.html -- 14.8 Кб -- 02.10.2012
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45. http://www.jsc.nasa.gov/history/oral_histories/DeiterichCF/DeiterichCF_Bio.pdf
NASA JOHNSON SPACE CENTER ORAL HISTORY PROJECT BIOGRAPHICAL DATA SHEET NAME: Charles F. Deiterich O RAL H ISTORY: 28 February 2006 EDUCATIONAL BACKGROUND: B.A. in Physics/Mathematics, University of St. Thomas, Houston , Texas , 1960 M.S. in Physical Science, University of Houston Clear Lake, Clear Lake, Texas , 1984 PRE-NASA EXPERIENCE: Electro/Mechanical Engineer, Transport Flight Systems, Vecto Instrument Corporation, ...
[ Текст ]  Ссылки http://www.jsc.nasa.gov/history/oral_histories/DeiterichCF/DeiterichCF_Bio.pdf -- 28.7 Кб -- 24.01.2007
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46. http://selena.sai.msu.ru/Pug/Publications/m44_70_pugacheva.pdf
THE PHOTOMETRIC RESEARCHS OF THE MERCURY'S SURFACE BY MEANS OF DIGITAL MODELS. ... The surface brightness of Mercury was measured Danjon (1933, 1949, 1953) and Harris (1961) in phase angle 3o-123o. The analysis of the various data of the integral photometric gives the results of determination of the main photometric constants for Mercury. ... THE PHOTOMETRIC RESEARCHS OF THE MERCURY'S SURFACE: S.G. Pugacheva The surface brightness of the Mercurian images was established on the geologic map Mercury. ...
[ Текст ]  Ссылки http://selena.sai.msu.ru/Pug/Publications/m44_70_pugacheva.pdf -- 205.0 Кб -- 25.02.2009
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47. Theoretical Astrophysics Department
. Cosmology . Very Early Universe . Cosmic Microwave Background Anisotropy . Dark Matter Models . Large Scale Structure . High Energy Astrophysics . Active Galactic Nuclei . Astrophysics of Compact Objects . Accretion Disks . Scientific Staff:
[ Сохраненная копия ]  Ссылки http://www.asc.rssi.ru/mdiv/tad/tad.htm -- 1.8 Кб -- 04.12.1997
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48. Iowa Robotic Telescope Facilities
... Iowa Robotic Telescope | ... Talon is based on OCAAS, a software suite developed by software engineer Elwood Downey ( Clear Sky Institute ) for use at the University of Iowa ?s first remote facility (the ATF, or Automated Telescope Facility). ... XObservatory : Telescope Control Interface . ... This program calls upon and coordinates much of the interrelated portions of the Talon architecture, and forms the primary control panel for the telescope, dome, and peripheral systems when used locally. ...
[ Сохраненная копия ]  Ссылки http://vega.inp.nsk.su/~inest/Talon(OCAAS)/Iowa%20Robotic%20Telescope%20Facilities.htm -- 37.9 Кб -- 25.01.2006
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49. Multiwavelength Study of Mira Ceti-Type Variable Stars
... There are preliminary series of photometric and radio spectral observations of the above-mentioned stars, archival data on the light curves of the stars, results of the search for OH and H 2 O maser emission in IRAS point sources that possess the IR parameters similar to Miras. ... The aim is a detailed study of the maser emission variability. ... In 1996-1997, astronomical observations of Mira Ceti-type stars (miras) were carried out in three spectral ranges: optical, infrared, and radio. ...
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/~gmr/miras.html -- 13.9 Кб -- 25.11.2015
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50. http://www.issp.ac.ru/lsc/files/Laue%20optics_Nuclear%20instrumetnts%20and%20methods_2009.pdf
... Today, Laue lenses have demonstrated their capability of focusing gamma-rays in the 100 keV­1 MeV domain, enabling the possibility of building a new generation of instruments for which sensitive area is decoupled from collecting area. ... Then the state of the art of development of Laue lens elementary constituents--metallic or semiconductor crystals--is given before tackling the heart of subject of this paper with the presentation of a Laue lens response. ...
[ Текст ]  Ссылки http://www.issp.ac.ru/lsc/files/Laue%20optics_Nuclear%20instrumetnts%20and%20methods_2009.pdf -- 359.3 Кб -- 09.02.2012
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51. 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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52. SAI Space Monitoring Laboratory
Lab . Main page News People . ASA . Master . Master net Homepage . ... Lomonosov Moscow State University Sternberg Astronomical Institute . ... MASTER . ... Lomonosov (ShOK) . ... About Space Monitoring Laboratory, scientific directions, instruments, contacts . People, who work in lab . Latest news and news archive . ... Gamma-Ray Bursts observations . Theory of Gamma-Ray Burst formation . ... MASTER (Global Robotic optical monitoring system) . ... All news ...
[ Сохраненная копия ]  Ссылки http://master.sai.msu.ru/en/ -- 8.2 Кб -- 09.04.2016
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53. Limiting Magnitude Table
DISCLAIMER: The larger the aperture, the more light a telescope will gather and the fainter the object you can see. Here is a range of magnitudes you might expect to see. Given excellent sky conditions and good optics, a well trained eye can sometimes add up to 0.8 magnitude to these values. Limiting Magnitude depends on much more than the instruments aperture. ... One formula is for aperture in inches the other is for aperture in millimeters. ... Aperture (inches) . ... 15.2 . ...
[ Сохраненная копия ]  Ссылки http://www.wro.org/ras/matto/limiting_magnitude_table.htm -- 9.6 Кб -- 18.08.2005
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54. 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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55. 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 . ...
[ Сохраненная копия ]  Ссылки http://www.puldb.ru/db/plates/index.php -- 6.7 Кб -- 01.10.2012
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56. http://www.armaghplanet.com/pdf/AstroTopics/Measuring%20the%20Universe/Parallax.pdf
... After all we cannot send a probe to the star Altair to confirm that it is 17 light years away. ... The "Bessel determined that the star 61 Cygni was about ten light years away" Earth goes around the Sun in one year, so in six month it is in the opposite position in its orbit. ... In 1838 Bessel determined that the star 61 Cygni had a parallax of 0.314 arcseconds and therefore the star was about ten light years away (today the distance is more precisely measured to be 11.4 light years). ...
[ Текст ]  Ссылки http://www.armaghplanet.com/pdf/AstroTopics/Measuring%20the%20Universe/Parallax.pdf -- 102.6 Кб -- 20.09.2011
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57. Project Space Hotel
... Space flight . ... Space Hotel . ... The program of deployment of small orbital station (SOS) consisting of a family of spacecrafts and module-spacecrafts represents a consecutive realization of flight scenarios with consecutive building up of functions. ... Scenario 1 - the regular and revised spacecrafts of class "Soyuz" - TMSC and MNMSC (MNMSC-cargo, MNMSC-MR) are used, pls. see fig fig.8 . ... The terms of transition to this scenario are determined by terms of readiness of one or another module....
[ Сохраненная копия ]  Ссылки http://www.atlasaerospace.net/eng/spacehotel-exp.htm -- 39.4 Кб -- 09.04.2016
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58. Ли Оптика
. ИЗГОТОВЛЕНИЕ . АСТРОНОМИЧЕСКИХ ПРИБОРОВ И ОПТИКИ . ДЛЯ ЛЮБИТЕЛЕЙ И ПРОФЕССИОНАЛОВ . FABRICATION . OF ASTRONOMICAL INSTRUMENTS AND OPTICS . FOR AMATEURS AND PROFESSIONALS . о компании . оптика . телескопы . контакт . 300 мм телескоп Ньютона на установке Добсона . about company . optics . telescope . contact . Тел./Факс.536-89-22 .
[ Сохраненная копия ]  Ссылки http://www.lioptics.narod.ru/ -- 3.4 Кб -- 09.04.2016
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59. Equations of Mathematical Physics
There are many ordinary/partial differential equations/systems describing various phenomena in physics, mechanics, chemistry, biology, sociology, etc. ... Prerequisites: 1 semester "Advanced Calculus", 1 semester "Linear Algebra". Optional: 2 semester "Advanced Calculus", 2 semester "Linear Algebra", 1 semester "Functions of Complex Variables", elements of the functional analysis and the ordinary differential equations theory. ... Laplace transform for linear differential equations . ...
[ Сохраненная копия ]  Ссылки http://www.mccme.ru/mathinmoscow/courses/view.php?name=Equations%20of%20Mathematical%20Physics.htm -- 4.5 Кб -- 01.03.2014
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60. Speckle polarimeter
... Speckle polarimeter (previosly known as Multimode Fast Camera MFC) is an instrument which will implement several observational methods of astronomy in visible (BVRI bands): speckle interferometry, polarimetry, speckle polarimetry (including polaroastrometry), and fast photometry. The speckle polarimeter will be installed in one of auxiliary Nasmyth ports of 2.5 m telescope of Sternberg Astronomical Institute. Speckle interferometry. ... Tests of speckle polarimeter at 2.5 m telescope. ...
[ Сохраненная копия ]  Ссылки http://lnfm1.sai.msu.ru/kgo/mfc_en.php -- 26.3 Кб -- 09.04.2016
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