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41. Accuracy of World positional CCD observations of the numbered minor planets
... Contact A Problem of an estimation of accuracy of the asteroid CCD observations . The Minor Planet Center supported by the Interntional Astronomical Union is the main office for keeping observational data of the small Solar System bodies and their investigations. ... At Pulkovo Observatory we are estimating an accuracy of the CCD asteroid observations obtained by amateurs and professional astronomers all over the World using the MPC database. ...
[ Сохраненная копия ]  Ссылки http://www.accuracy.puldb.ru/PROBLEM.HTM -- 3.9 Кб -- 05.12.2007
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42. Radioastrophysical Observatory ISTP RAS SB
RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . General information Main characteristics of the Radio telescope Observing programs General view of the antenna array Main research areas Principle of generation of radio images Radio telescope 's beam Receiving systems Main characteristics of the base receiving-recording complex Calibrations Data archive and databases Publication SSRT - Siberian Solar Radio Telescope . ...
[ Сохраненная копия ]  Ссылки http://ssrt.iszf.irk.ru/rad11en.shtml -- 17.2 Кб -- 27.02.2014
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43. S.P.Korolev RSC Energia - LAUNCHERS
Geophysical rocket R-11A . ... Rocket R-11A has been designed to take measurements of atmospheric pressure at different altitudes from 60 to 160 km, define optical properties of upper atmospheric layers, measure concentration of positive ions, record a number of the container collisions with micrometeorites. Rocket P-11A was first launched from the Novaya Zemlya in October 1958. The rocket reached an altitude of 103 km. ... SEA LAUNCH . ... Official WEB-site of S.P.Korolev RSC Energia . ...
[ Сохраненная копия ]  Ссылки http://www.energia.ru/english/energia/launchers/rocket-r11a.html -- 8.5 Кб -- 02.10.2012
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44. Marc White - Astrophysicist - The Australian National University
Marc White . ... Research . ... The outflows driven by forming protostars provide important clues to the nature of the star formation process. My research focuses on observations and analysis of the outflows driven by actively-accreting protostars. ... How are the outflows being driven? ... Built by my home institution, The Research School of Astronomy and Astrophysics of The Australian National University, NIFS is a fantastic instrument for doing protostellar outflow work. ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~mwhite/research.php -- 7.8 Кб -- 27.02.2014
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45. The COOC Criterion (Criterion of Observations versus Calculations)
... In order to compare the number of different evolutionary stages obtained and X-ray luminosity of the chosen X-ray sources with the observed galactic values we use the sum of C/O+O/C , where C and O are the calculated and observed values of a given binary type, respectively. If we make comparison for a number of different binary species (for example, we compare the number of CV, number of X-ray pulsars,   total X-ray luminosity of LMXB, etc.), we write this criterion in the form: . ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node43.html -- 5.0 Кб -- 26.02.1997
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46. atmos 3.0 page
The most up-to-date information related to atmos 3.0 are collected here due to constantly increasing interest to MASS/DIMM processing software... atmos 3.0 is still beta , so the latest version is 2.97.5 (there is also 2.98.x branch which absorbs new features) . ... M' line: . ... free seeing and its relative error . ... dimm seeing and its relative error (if dimm data are present, zeros otherwise) . ... dimm turbulence power and its relative error (if dimm data are present, zeros otherwise) . ...
[ Сохраненная копия ]  Ссылки http://curl.sai.msu.ru/~matwey/atmos/ -- 6.8 Кб -- 05.02.2016
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47. Program features
... Program: . ... There are twenty one math courses and two theoretical computer science courses. Besides math and computer science courses, a Russian language course, courses in Russian history, history of science and Russian literature (in English) are offered. ... However, we are aware that most students in the Math in Moscow program do not have as much math problem solving experience as Russian students of the same age. ... One "Math in Moscow" course transfers as three or four semester hours. ...
[ Сохраненная копия ]  Ссылки http://www.mccme.ru/mathinmoscow/?page=3 -- 16.8 Кб -- 10.04.2016
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48. http://www.astro.louisville.edu/shared_skies/archive/select/unusual/hoags_object/20130412/hoags_object_wikipedia_20130422.pdf
... Courtesy of NASA/ESA Observation data (J2000 epoch) Constellation Right ascension Declination Redshift Distance Type Serpens Caput 15h 17m 14.4s[] +21° 35 08[] 12,740±50 km/s[][1] 600±30 Mly (183±8 Mpc)[1] SA0(r) [citation needed ] [a] Apparent dimensions (V) 0.28 в 0.28[] Apparent magnitude (V) 16.0[] Notable features Ring galaxy Other designations PGC 54559,[] PRC D-51[] See also: Galaxy, List of galaxies Hoag's Object is a non-typical galaxy of the type known as a ring galaxy. ...
[ Текст ]  Ссылки http://www.astro.louisville.edu/shared_skies/archive/select/unusual/hoags_object/20130412/hoags_object_wikipedia_20130422.pdf -- 498.8 Кб -- 22.04.2013
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49. 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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50. astro-ph
... Aims: Today, large ground-based instruments, like VISIR on the VLT, providing diffraction-limited (about 0.3 arcsec) images in the mid-infrared where strong PAH features appear enable us to see the flaring structure of the disks around Herbig Ae stars. Although great progress has been made in modelling the disk with radiative transfer models able to reproduce the spectral energy distribution (SED) of Herbig Ae stars, the constraints brought by images have not been yet fully exploited. ...
[ Сохраненная копия ]  Ссылки http://vo.astronet.ru/arxiv/?get_articles=1&author=E -- 10.4 Кб -- 12.09.2010
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51. http://xray.sai.msu.ru/~polar/sci_rev/1012.html
... Authors: Nikku Madhusudhan et al. arxiv:1012.1218 Наблюдения рентгеновского пульсара MAXI J1409-619 на BeppoSAX в спокойном состоянии: открытие циклотронных линий (BeppoSAX observations of the X-ray pulsar MAXI J1409-619 in low state: discovery of cyclotron resonance features) . ... Authors: Christoph Mordasini et al. миниобзор arxiv:1012.2932 Магнитное поле нашей Галактики (The Magnetic Field of the Milky Way Galaxy) . Authors: Jo-Anne Brown . ... Authors: William E. Harris ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~polar/sci_rev/1012.html -- 3.2 Кб -- 06.01.2011
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/astro-ph/1012.html -- 3.2 Кб -- 27.02.2014
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52. Departement of Quantum Astrophysics
. Departement of Quantum Astrophysics . Head: Kurt V.G. , Prof. ultraviolet spectroscopy of planetary upper atmospheres and interplanetary/interstellar medium; . observations of gamma-bursts and optical identification of their sources; . long-base optical interferometry. Staff: .
[ Сохраненная копия ]  Ссылки http://www.asc.rssi.ru/mdiv/qad/qad.htm -- 1.9 Кб -- 04.12.1997
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53. Pulkovo Databases
System of astrometric databases of Pulkovo observatory. 26-inch refractor . Pulkovo system of astrometric databases consists of three databases, which contain results of processing photographic and CCD observations, obtained with the 26-inch refractor and the Normal astrograph of Pulkovo observatory. Pulkovo photographic catalogs: Pul-2, Pul-3 (Pul-3 SE), Pul ERS . Results of photographic and CCD observations of Solar system objects . ... Normal Astrograph ...
[ Сохраненная копия ]  Ссылки http://www.puldb.ru/db/help1.php -- 4.3 Кб -- 01.10.2012
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54. Comet Observation Home Page (Chernogolovka)
... Copyrightї1997 Bob Yen (byen@ix.netcom.com) (http://www.comet-track.com/hb/hb.html) . ... Information on Comet Hale-Bopp for the Non-Astronomer Hale-Bopp rotates about twice a day (3/14/97) . ... The Comet Observation Home Page was been selected to receive the Griffith Observatory Star Award for the week of February 2 - 8, 1997 for excellence in promoting astronomy to the public through the World Wide Web. ... Typically, about 1,000 individual users/computers access this page every day. ...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/univer/astro/comets/ -- 9.6 Кб -- 11.04.2001
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55. http://hea.iki.rssi.ru/integral06/papers/F36_Del_Santo02-04May07_15:17:45.pdf
... Classified as a persistent source, on 2004 it showed a quiescent-like state. ... We present the long term temporal behaviour of 1E 1740.7­2942 observed by INTEGRAL and RXTE in 2004 and 2005, as well as preliminary results on possible spectral transitions. ... 1E 1740.7­2942 RXTE/PCA ligh curve based on short pointings in the energy range 6­12 keV. given. ... Our 2005 simultaneous INTEGRAL and RXTE observations were performed in high flux levels; as expected 1E 1740.7­2942 was in its Low/Hard state. ...
[ Текст ]  Ссылки http://hea.iki.rssi.ru/integral06/papers/F36_Del_Santo02-04May07_15:17:45.pdf -- 344.4 Кб -- 04.05.2007
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56. http://lnfm1.sai.msu.ru/neb/nss/coorb/coorb_anno.doc
OBSERVATIONS OF COORBITAL SATELLITES OF SATURN Emel'yanov N., Varfolomeev M. Sternberg State Astronomical Institute, Moscow, e-mail : emelia@sai.msu.ru Institut de MИcanique CИleste et de Calcul des иphИmИrides, Paris, e-mail : emelia@imcce.fr Abstract. To improve the orbital parameters and masses of coorbital satellites of Saturn, Janus and Epimetheus, new observations of these satellites are necessary. ... IN: Saturn. ... New observations of Saturn's coorbital satellites" - Icarus. ...
[ Текст ]  Ссылки http://lnfm1.sai.msu.ru/neb/nss/coorb/coorb_anno.doc -- 90.5 Кб -- 15.04.2007
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57. VISTA - Visible and Infrared Survey Telescope for Astronomy
... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...
[ Сохраненная копия ]  Ссылки http://www.vista.ac.uk/ -- 31.7 Кб -- 27.11.2014
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58. SINGULAR POINTS IN THE SOLAR CHROMOSPHERE
SINGULAR POINTS IN THE SOLAR CHROMOSPHERE . ... In the structure of the solar chromosphere, containing information on the configuration of the magnetic field, we have found and identified all the main types of the singular points ( see Fig. 1 ), which are known as inherent features of the 2-D vector field. ... The main types of the singular points are the node, the focus, the center, and the saddle. ... Singular point of the focus type in the solar chromosphere. ...
[ Сохраненная копия ]  Ссылки http://www.izmiran.rssi.ru/info/personalia/molodensky/spoints.html -- 8.2 Кб -- 11.12.2015
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59. Mid Scales Role
... ON THE ROLE OF LARGE-SCALE PLASMA IRREGULARITIES AT THE FINAL STAGE OF ANOMALOUS ABSOPTION DEVELOPING UNDER HF HEATING OF THE IONOSPHERE . ... Fig. ... With the aid of numerical statistical modeling based on multiple ray tracing it is shown that in presence of large-scale irregularities the reflected signal amplitude mean value is increased significantly. ... Dependence of the mean amplitude of the reflected from the ionosphere signal on the large-scale (10-50 km) electron density irregularity level...
[ Сохраненная копия ]  Ссылки http://ip.rsu.ru/~zabotin/posters/mid_sc/mid_sc.htm -- 11.1 Кб -- 02.02.2007
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60. Double Engine Fuels Star's Remarkable Nebula - Astronomy news
... Astronomy news . ... Double Engine Fuels Star's Remarkable Nebula . ESO has just released a stunning new image of a field of stars towards the constellation of Carina (the Keel). ... Interactions in this double system, surrounded by a dusty disc, may be the engine fuelling the star s remarkable nebula. The new image, showing a very rich field of stars towards the Carina arm of the Milky Way, is centred on the star HD 87643, a member of the exotic class of B[e] stars [1]. ...
[ Сохраненная копия ]  Ссылки http://www.tesis.lebedev.ru/en/astronomy_news.html?did=1936 -- 14.0 Кб -- 11.04.2016
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