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http://uranus.sai.msu.ru/~seif/ST12_apj_747_2_99.pdf.
http://uranus.sai.msu.ru/~seif/ST12_apj_747_2_99.pdf.
41. Current Weather Conditions
... February: 25 out of 28 days with mesureable precipitation . March 1-12: 6 degrees below normal average temperature . ... March: Average high temperatue 6 degrees below normal. 11 days with highes below 50 . ... April 16: Record high = 77 . ... June 9: Record Low - 34 . ... August 7; High = 65; rain =0.41 inches (both close to records) . August 11: Record Low maximum of 68. ... Sept 2: Record low of 38 . Sept 28: Record Low - 31 (all time record low for the month of September) . ...
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Ссылки http://zebu.uoregon.edu/1999w.html -- 2.9 Кб -- 02.09.2000
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42. If neutron stars don't produce energy from fusion, like normal stars, how can
... Star Atlas . ... stars . ... If neutron stars don't produce energy from fusion, like normal stars, how can they shine in visible light? ... Although it is true that neutron stars have, for the most part, consumed all their internal thermonuclear fuel, they tap into other energy sources to produce light. Indeed, neutron stars are remarkably "resourceful" and employ a variety of physical mechanisms to make themselves visible.A newborn neutron star is incredibly hot ? ... Atlas of the Stars . ...
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Ссылки http://www.astronomy.com/magazine/ask-astro/2005/03/if-neutron-stars-dont-produce-energy-from-fusion-like-normal-stars-how-can-they-shine-in-visible-light -- 63.4 Кб -- 10.04.2016
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43. 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. ...
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Ссылки http://www.mso.anu.edu.au/~mwhite/research.php -- 7.8 Кб -- 27.02.2014
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44. http://www.asc.rssi.ru/RadioAstron/publications/articles/cr_2014,52,391.pdf
... Numerical Modeling of RadioAstron SRT Temperature Deformations M. Yu. Arkhipov, I. S. Vinogradov, S. B. Novikov, and S. D. Fedorchuk Astro Space Center, Lebedev Physical Institute of the Russian Academy of Sciences, Moscow, Russia e mail: rusengineer@mail.ru Received December 16, 2013 Abstract--The results of modeling the thermal deformations of a space radio telescope's reflecting surface are presented in the paper. ...
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Ссылки http://www.asc.rssi.ru/RadioAstron/publications/articles/cr_2014,52,391.pdf -- 437.2 Кб -- 07.10.2014
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45. ASP: Astronomy in the News
Mercury Spring 2010 Table of Contents . This artist s impression shows the transiting exoplanet Corot-9b. Credit: ESO / L. Cal ada. First Temperate Exoplanet . ... Combining observations from the CoRoT satellite and the ESO HARPS instrument, astronomers have discovered the first . ... Designated Corot-9b, the . ... If you enjoyed this excerpt from a feature article and would like to receive our quarterly Mercury magazine, we invite you to join the ASP and receive 4 issues a year. ...
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Ссылки http://www.astrosociety.org/pubs/mercury/39_02/astronews.html -- 7.5 Кб -- 02.10.2012
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46. The NMW survey homepage
NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...
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47. Linear polarization: wavelength dependence
... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...
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Ссылки http://www.astro.spbu.ru/DOP/8-GLIB/ASTNOTES/node7.html -- 18.9 Кб -- 19.11.2010
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48. http://selena.sai.msu.ru/Bus/Publications/ACM08(Bus).pdf
Asteroids, Comets, Meteors (2008) 8010.pdf SPECTRAL SIGNS OF CARBONACEOUS CHONDRITIC MATERIAL ON (21) LUTETIA V.V. Busarev, Sternberg Astronomical Institute (SAI), Moscow University, Universitetskij pr., ... We have discovered considerable variations in the continuum slope and shape of the visible-range reflectance spectra of the asteroid with rotation in November 2004 (4/5, 5/6 and 7/8) and March 2006 (3/4). ... Resulting normalized (at 0.55 m) and smoothed reflectance spectra are shown in Fig. ...
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Ссылки http://selena.sai.msu.ru/Bus/Publications/ACM08(Bus).pdf -- 120.1 Кб -- 17.02.2009
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49. http://www.izmiran.rssi.ru/~obridko/papers/279engl.pdf
... Relation between the Structure of the Large-Scale Solar Magnetic Field in the Activity Cycles and IMF Governing Geomagnetic Activity V. N. Obridko , S. A. Golyshev, and A. E. Levitin Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation, Russian Academy of ... oblast, 142190 Russia Received September 30, 2003; in final form, December 19, 2003 Abstract--It has been corroborated that the sign and amplitude of the annual ...
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Ссылки http://www.izmiran.rssi.ru/~obridko/papers/279engl.pdf -- 141.8 Кб -- 14.03.2011
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50. H2O maser spectral data.
H 2 O maser sources spectral data at 22 GHz. I began this project 27.08.1998 for displaying spectral data at 22 GHz of water maser. While data will concerning in base Puschino many year (1979-1998 yy) regular observations of sample of these sources. Sources . R.a. (1950.0) . ... The figures with many years spectral data (day-month-year) . The behavior of flux . The behavior of spectral components . ... All spectra 1981-94 . ... The some spectral component: many year behavior . ...
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Ссылки http://astra.prao.psn.ru/SAM/ENG/h2o_data.htm -- 4.9 Кб -- 16.02.2005
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51. COSMIC RAY Observation
Cosmic Ray laboratory of . ... Neutron Monitor (Cosmic Ray Observations) . is situated in Irkutsk (Russia) . ... Height - location above sea level . ... Height: . ... For recording the CR (Cosmic Rays) neutron component at Irkutsk, . neutron monitor NM-64 is used, which is an installation with 18 two-meter proportional counters filled with BF 3 (boron trifluoride gas) in which the B 10 90 per cent of the total boron. ... The neutron monitor is located at 475m above sea level. ...
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Ссылки http://cgm.iszf.irk.ru/irkt/about.htm -- 3.9 Кб -- 10.01.2005
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52. Scientific.ru Альтернативный форум
Альтернативный форум . Scientific.ru Все форумы . ... Chernov V.M. Non-Archimedian Normalized Fields and Аlgorithms for Two-Dimensional Discrete Fourier Transform. Pattern Reсogn. and Image Analysis.- ... Чернов В. М. О точности вычисления дискретной круговой свертки в нормированных полях. ... Чернов В.М. О дискретном "метапреобразовании" в кольце аделей глобального поля. ... Chernov V.M.,Shabashev A.V. Non-Archimedian normalized fields in texture analysis tasks. ... V.M.Chernov. ...
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Ссылки http://www.scientific.ru/dforum/altern/1121661815 -- 14.7 Кб -- 11.04.2016
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53. Circular Polarization
Abstract -- The strengths of magnetic fields in interstellar gas clouds are obtained through observations of the circular polarization of spectral line radiation. ... To infer information about these irregularities from the observational data, we develop statistical relationships between the rms values of the irregular component of the magnetic field and spatial variations in the circular polarization of the spectral line radiation. ...
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Ссылки http://www.inasan.rssi.ru/~dwiebe/abstracts/circular.html -- 2.8 Кб -- 27.09.2012
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54. http://xray.sai.msu.ru/~polar/sci_rev/1001.html
... Authors: Z. Paragi et al. arxiv:1001.4538 Семь лет WMAP. ... Authors: Thomas P. Robitaille, Barbara A. Whitney . ... Authors: The ACT Collaboration: J. W. Fowler et al. arxiv:1001.2017 Пространственно разрешенная спектроскопия экзопланеты HR 8799 c (Spatially resolved spectroscopy of the exoplanet HR 8799 c) . ... arxiv:1001.1738 SDSS J1254+0846: двойной квазар, застигнутый в момент слияния (Title: SDSS J1254+0846: A Binary Quasar Caught in the Act of Merging) . ... Authors: Douglas A. Caldwell et...
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Ссылки http://xray.sai.msu.ru/~polar/sci_rev/1001.html -- 4.2 Кб -- 02.02.2010
[ Сохраненная копия ] Ссылки http://astro.uni-altai.ru/astro-ph/1001.html -- 4.2 Кб -- 27.02.2014
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55. East Siberian Center for the Earth's Ionosphere Research. SW radiosignal
Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... The algorithm and appropriate program for decametric radiosignal propagation conditions prediction for paths from 500 to 9000 km have been developed at ISTP SB on the basis of normal wave method (AltyntsevaB.I,Iliyin N.V., Kurkin V.I. and others //Decameters channel simulation on the base of normal wave method . ... Solar activity indices are chosen automatically from the prediction date from the database . ...
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Ссылки http://rp.iszf.irk.ru/esceir/lchmen/predicten.htm -- 8.0 Кб -- 02.06.2001
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56. Specialized space training (SST)
... Space flight . Crew training . ... Space camp . ... acquiring practical habits and skills of performing all the flight operations envisaged for a flight participant; . maintaining and honing professionally required qualities and skills for a successful activity in conditions of effect of adverse factors of a space flight, as well . ... preparing for the activity outside the spacecraft; . ... preparing for professional activity in conditions of effect of the space flight factors; . ...
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Ссылки http://www.atlasaerospace.net/eng/podgotovka-skp.htm -- 31.6 Кб -- 09.04.2016
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57. http://sn.sai.msu.ru/~sil/preprints/iau254sil.pdf
The Galaxy Disk in Cosmological Context Proceedings IAU Symposium No. ... The presence of exponential bulges and anti-truncated disks has been noticed in many lenticular galaxies. ... Among our findings in unbarred spiral galaxies, only one galaxy, NGC 5533, has a LSB outer disk (Sil'chenko et al. ... In the frame of this model, the Exponential bulges and antitruncated disks 5 inner disk must be more bright and compact than the usual large-scale stellar disks of spiral galaxies are. ...
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Ссылки http://sn.sai.msu.ru/~sil/preprints/iau254sil.pdf -- 285.3 Кб -- 23.01.2010
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58. Supernova 2002dv and 2002eg in UGC 11486
Supernova 2002dv and 2002eg in UGC 11486 . This page is devoted to information on Supernova 2002dv and Supernova 2002eg in UGC 11486 Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . ... Ella Sanders discovered this one, the thrid double SN in four months, almost a stastical impossibility. ... SNWeb has a 2002dv page . ... Ella Sanders 2002eg images page 1 and 2002eg images page 2 . ... 2002/07/01.4 . ... Ella Sanders image . ...
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Ссылки http://www.sai.msu.su/mirrors/isn/sn2002/sn2002dv.html -- 10.2 Кб -- 22.12.2007
[ Сохраненная копия ] Ссылки http://www.rochesterastronomy.org/sn2002/sn2002dv.html -- 10.2 Кб -- 19.04.2014
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[ Сохраненная копия ] Ссылки http://www.rochesterastronomy.org/sn2002/sn2002dv.html -- 10.2 Кб -- 19.04.2014
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59. ColorThresholder (ImageJ API)
... Class . ... public class ColorThresholder . ... Nested classes/interfaces inherited from class java.awt.Frame . ... Nested classes/interfaces inherited from class java.awt.Window . ... Nested classes/interfaces inherited from class java.awt.Container . ... Nested classes/interfaces inherited from class java.awt.Component . ... void . ... public void getLab ( ImageProcessor ip, byte[] L, byte[] a, byte[] b) . public void getYUV ( ImageProcessor ip, byte[] Y, byte[] U, byte[] V) . ...
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Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/plugin/frame/ColorThresholder.html -- 35.0 Кб -- 02.12.2010
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60. source comment
... The derived position here agrees with the position from recent ATCA observations, RA=15h 01m 34.74s, Dec=39 18 39.2" (Tasker, private communication) which found the source unresolved. Because of the relatively large position offset, the reality of the fainter component 0.12" to the west is somewhat in doubt. However, the ATCA centroid position is offset by 0.3" to the south-east of the VLBA position, suggesting that the faint component may be part of more extended structure. ...
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Ссылки http://www.vsop.isas.ac.jp/VLBApls/J1501-3918.comment.htm -- 1.8 Кб -- 16.10.2000
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