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1. Optical turbulence
... General information . ... Staff . Research staff . Technical, administrative & librarian staff . ... Staff in alphabetic order . Research . Adaptive Optics . ... High energy . ... Projects . ... General interest seminars . ... Information . ... Historical highlights . Historical research . ... The Adaptive Optics and Optical Turbulence groups are part of the research pole of "High angular resolution techniques for ground-based observations" of the Arcetri Astrophysical Observatory. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/en/research/optical-turbulence -- 24.5 Кб -- 09.04.2016
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2. Index of /txt/2009/presentations/Turbulence and chaos
... Parent Directory - Artemyev.ppt 30-Mar-2009 19:55 4.2M Dolgonosov.rar 30-Mar-2009 19:55 5.5M Ephimov.pps 30-Mar-2009 19:55 11M Frank.pdf 30-Mar-2009 19:55 3.7M Golovchanskaya.ppt 30-Mar-2009 19:55 6.3M Grigorenko.ppt 30-Mar-2009 19:55 6.4M Knyazeva.ppt 30-Mar-2009 19:55 494K Kozelov.ppt 30-Mar-2009 19:55 1.3M Kropotkin.ppt 30-Mar-2009 19:55 3.0M Lutzenko.ppt 30-Mar-2009 19:55 3.1M Makarenko1.ppt ...
[ Сохраненная копия ]  Ссылки http://solarwind.cosmos.ru/txt/2009/presentations/Turbulence%20and%20chaos/ -- 3.6 Кб -- 01.10.2012
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3. Астронет > AO tutorial 1: turbulence
... Астронет | ... планета Астронет | ... BACK . ... Астигматизм . ... Астигм. 5-го пор. ... Публикации с ключевыми словами: адаптивная оптика - атмосфера - волновой фронт . Публикации со словами: адаптивная оптика - атмосфера - волновой фронт . ... Циркуляция атмосферы . Циркуляция атмосферы, общая . Атмосферная циркуляция . ... Нептун через адаптивную оптику . Все публикации на ту же тему >> . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/msg/1205112/part1/zernike.html -- 22.6 Кб -- 08.04.2005
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4. Alexei Kritsuk's Home Page
... Project page . ... Project workpage . Turbulence in the Multiphase Interstellar Medium . Project I | ... Project highlight | ... Towards simulating turbulence with adaptive meshes . ... A. Kritsuk, P. Padoan, M. Norman . ... A. Kritsuk M. Norman . ... A. Kritsuk, M. Norman, P. Padoan . astro-ph/0411626 | ... P. Padoan, A. Kritsuk, M. Norman, A. Nordlund . ... Introducing Enzo, an AMR Cosmology Application . B. O'Shea, G. Bryan, J. Bordner, M. Norman, T. Abel, R. Harkness, A. Kritsuk . ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/staff/agk/ -- 10.8 Кб -- 19.11.2010
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5. Scholarly Pursuits
. Int. J. Multiphase Flow 21, 467-483, 1995. In preparation, 1995. Int. J. Multiphase Flow 20, 415-437, 1994. Phys. Fluids 6, 3109-3115, 1994. Studies in Turbulence (Gatski, Sarkar, Speziale Eds.) 461-483, Springer-Verlag 1992. AIAA Journ. 28, 106-112, 1990. Jacques Lewalle, jlewalle@syr.edu
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/~vab/Wavelet.rsc/Tutor.dir/flows.html -- 3.7 Кб -- 12.04.1998
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6. http://site2010.sai.msu.ru/static/doc/ATokovinin_site2010.pdf
Surface-layer turbulence measurements with lunar scintillometer Idea of the method Hardware & software Campaigns & results New horizons Andrei Tokovinin NOAO/CTIO Kislovodsk Oct. 2010 1 Turbulence measurement from scintillation of extended sources Moon's angular diameter =0.5 deg Correlated scintillation for b > z z=10m b=0.1m z=100m b=1m z=10km b=100m BI(b) = W(b,z) Cn2(z)dz Weighting functions zW(z) for b=0...0.4m and d=1cm 2 Kislovodsk Oct. ... 2010 12 Paranal: October 14, 2008 Kislovodsk Oct. ...
[ Текст ]  Ссылки http://site2010.sai.msu.ru/static/doc/ATokovinin_site2010.pdf -- 2798.2 Кб -- 18.10.2010
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7. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . The more we explore our Galaxy the more difficult it becomes to find static initial states. This leads us to study molecular clouds as dynamic in which initial conditions are neither prescribed or necessary. And this leads us to a new emerging paradigm which solves many of the nagging problems of the last two decades. The birth of stars is regulated by supersonic turbulence and its interplay with gravity. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/research/turbulence.html -- 6.6 Кб -- 08.03.2013
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8. Post-Detection Turbulence Compensation
... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australian Square Kilometre Array Pathfinder . Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . ... Visiting Parkes radio telescope . Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ... It is against the above background that the technique of `post-detection turbulence compensation' has been developed (Primot et al. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/14_2/robertson/paper/node2.html -- 53.0 Кб -- 08.04.2016
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9. http://curl.sai.msu.ru/mass/download/doc/res2007eng.pdf
Preliminary results of astroclimate parameters measurements at the Sternberg 2.5m telescope installation site V.Kornilov, N.Shatsky, S.Potanin, O.Voziakova, B.Safonov Moscow, 2008 Acknowledgements A.Belinskiy M.Kornilov A.Tokovinin M.Kuznetsov P.Kortunov E.Gorbovskoy SAI administration some SAI students Pulkovo solar station (KHSS) staff RFBR support MAVEG Gmbh Why to study optical turbulence and some other relevant ... Mean seeing by DIMM data for this night is 1''5. ...
[ Текст ]  Ссылки http://curl.sai.msu.ru/mass/download/doc/res2007eng.pdf -- 2802.3 Кб -- 23.03.2008
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10. Nonlinear Wave Processes in Plasma
Nonlinear harmonics in plasma. Nonlinear electromagnetic wave in plasma. ... Turbulence spectra. Wave- wave interaction. ... Brillouin back- scattering. Parametric instability. The balance equations. ... Wave- particle interaction in random phase approach. ... Stimulated scattering of waves by particles. Weak turbulence processes. Inverse energy cascade in plasma. ... Inverse scattering method. ... Nonlinear Schrodinger equation. ... Strong nonlinear 3- wave interaction. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/courses/nelin_hv_proc_u_pl_e.html -- 3.4 Кб -- 23.02.2005
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11. Galaxy sector, archive 1993
... 1993: . ... It was shown that the degree of the drop in turbulence depends on the magnetic field strength and the fact that it is completely suppressed at the field strengths of 4-5 kG. As a consequence, there arise the conditions of unimpeded diffusion of chemical elements under the influence of radiation pressure, so the degree of chemical anomalies depends on the magnetic field strength. ... Archive . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/Science/results/ar_galaxy/res1993.html -- 5.7 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/Doc-en/Science/results/ar_galaxy/res1993.html -- 5.7 Кб -- 10.04.2016
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12. 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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13. Mariner 5 solar wind problem finds answer: Turbulence doesn't go with the flow
... solar system . ... Observe the Solar System . ... Mariner 5 solar wind problem finds answer: Turbulence doesn't go with the flow . ... Research led by astrophysicists at the University of Warwick in Coventry, the United Kingdom, has resolved a 40-year-old problem with observations of turbulence in the solar wind first made by the probe Mariner 5. ... Our current understanding tells us that turbulence in the solar wind should not be affected by the speed and direction of travel of that solar wind. ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/news/2011/08/mariner-5-solar-wind-problem-finds-answer---turbulence-doesnt-go-with-the-flow -- 71.2 Кб -- 10.04.2016
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14. Dubovikov Mikhail Mikhailovich, Astro Space Center (ASC)
... Department Number . ... Astro Space Center . ... Telephone Number . 7(095) 333 3366 . FAX Number . 7(095) 333 2378 . ... dubovik@dpc.asc.rssi.ru ...
[ Сохраненная копия ]  Ссылки http://www.asc.rssi.ru/mdiv/people/mdubov.htm -- 2.3 Кб -- 04.12.1997
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15. astro-ph
... astro-ph . ... Aims: We aim for an understanding of the morphological and spectral properties of the supernova remnant RCW~86 and for insights into the production mechanism leading to the RCW~86 very high-energy gamma-ray emission. ... Studies of the morphological correlation between the 0.5-1~keV X-ray band, the 2-5~keV X-ray band, radio, and gamma-ray emissions have been performed as well as broadband modeling of the spectral energy distribution with two different emission models. ...
[ Сохраненная копия ]  Ссылки http://vo.astronet.ru/arxiv/?get_articles=1&author=S. -- 30.3 Кб -- 13.04.2016
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16. How Good An Astronomer Do You Need? - an Astronomy Net Education Forum Message
Astronomy Discussion Forums . Forums: . Atm ћ Astrophotography ћ Blackholes ћ Blackholes2 ћ CCD ћ Celestron ћ Domes ћ Education . ... How Good An Astronomer Do You Need? ... Post Message | ... So solar astronomy works with adaptive optics only when adaptive optics are not really needed to get good images, a negative result. ... www.astronomy.net . ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.net/forums/education/messages/104.shtml -- 15.1 Кб -- 09.04.2016
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17. ASP: The Face on Mars
If you go out tonight and look up at the full Moon, and you're like most people, you'll probably see the face of a man, or, alternatively, a rabbit superimposed on the bright disk of the Moon. ... When people look at the full Moon, they often see either a Man in the Moon (left) or a rabbit in the Moon (right). ... The Face on Mars is a naturally occurring rock outcropping that just happens to look like a face when lit from the side. ... The Face on Mars,'' Odyssey , October 1991, page 12. ...
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/edu/publications/tnl/25/face3.html -- 15.2 Кб -- 02.10.2012
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18. Modelling Astrophysical Turbulent Convection
... Numerical simulations of highly turbulent flows in astrophysics benefit greatly from recent advances in high performance computing. ... Figure: Perspective full domain view of vertical velocity at one instant in time in 3-D turbulent convection simulation ( ). ... Original PostScript figure (1496 kB) . ... Figure: Phase diagram of pointwise convective flux as function of the vertical velocity in a horizontal plane near midlayer for turbulent convection with , and , with . ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/brummelln.html -- 31.6 Кб -- 03.11.2000
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19. http://ssrt.iszf.irk.ru/html/public1991_ru.html
... Solar Physics,- 1991, - v. 135. Лубышев Б.И. , Смольков Г.Я. Результаты совместных наблюдений на ССРТ и РАТАН-600. ... Баландин А.Л., Кузнецова С.М., Обухов А.Г., Смольков Г.Я. Синтез радиоизображений Солнца при наблюдениях с ножевой диаграммой направленности. ... The Dynamics of Active region in microwave emission Proceedings of Symposium in Nobeyama Radioheliograph (26-28 Nov. ... The inversion of sign of the circular polarization of active region microwave emission t 5.2 cm wavelength. ...
[ Сохраненная копия ]  Ссылки http://ssrt.iszf.irk.ru/html/public1991_ru.html -- 8.9 Кб -- 20.12.2012
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20. http://hea.iki.rssi.ru/conf/hea2007/presentations.orig/25.12.07/medvedev.pdf
Mikhail Medvedev (University of Kansas) HEA- 2007 , IKI, Moscow Missing baryons in inter-cluster gas Afshordi, et al, 2007 , astro-ph/0612700 35% +/- 8% Sample of 260 clusters WMAP SZ 3yr data Compared with 11 simulated clusters Assumed: Universal NFW profile Self-similarity Isothermal gas Possible explanations Observed stellar mass in galaxies: ~ 10% (Lin, et al, ... Simulations indicate that the effect is small (Dolag, et al, 2004) Can account for ~1-2% missing mass at most ...
[ Текст ]  Ссылки http://hea.iki.rssi.ru/conf/hea2007/presentations.orig/25.12.07/medvedev.pdf -- 1403.9 Кб -- 29.12.2007
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