... Participants . ... The workshop will take place at two locations: the Independent University of Moscow (3 days) and the Steklov Mathematical Institute (2 days). ... The registration fee is 150 USD for foreign participants (paid upon arrival by those who can cover it from their grants or institutions) and 3000 roubles for participants from the FSU (also paid for those who can cover it from their grants). This covers also the welcome party and the conference dinner. ...

... Email: chaos@mail.cplire.ru Abstract - In this report, we investigate phenomena on the edge of spatially uniform chaotic mode and spatial temporal chaos in a lattice of chaotic 1-D maps with only local connections. ... PACEMAKER-CONTROLLED MODEL As we have already found, global synchronization is impossible in large lattices of locally coupled chaotic elements (maps). ... This synchronous mode is also chaotic (= 0.52В0.69) and stable, it attracts the lattice maps from any initial conditions. ...

The new view on the population of Galactic open clusters A.E.Piskunov1, N.V.Kharchenko2, S.RЖser3, E.Schilbach3, R.-D.Scholz4 1 2 3 4 Institute of Astronomy, Moscow, Russia Main Astronomical ... Observatory, Kiev, Ukraine Astronomisches Rechen-Institut, Heidelberg, Germany Astrophysikalisches Institut Potsdam, Germany What are open clusters and what do they teach us Groups of Population I ... Cluster complexes: OCC-1 = Gould's Belt cluster complex? ...

... Cluster Antares . ... Dual Intel Xeon 2.4 GHz, RAM 4GB, HDD 36GB + 73 GB RAID 0 массив . Сервер приложений (Linux) - IBM Intel Xeon 2.8 GHz, RAM 4 GB . Сервер приложений(Windows 2003 Server) - IBM Intel Xeon 3.2 GHz, RAM 4 GB . ... Dual dedicated connectivity: 100MBit/s + 1GBit/s. PVM 3.4.6, Atlas, MPI (MPICH2), HPL, PGI CDK (HPF) . GPU сервер "Tesla" : AMD Phenom (4 cores) + Nvidia Tesla C1060 GPU . ... Intel C++ compiler . ... Intel Cluster Toolkit Compiler Edition for Linux 3.2 . ...

... B.V. Somov . head of the department . ... room 80 . ... senior research felow . ... research felow . ... research fellow . ... Our department performes the following most perspective studies: . Special analytical and numerical experimental investigations of the solar plasma involved in the magnetic reconnection process at the Sun. ... Head of the seminar: Prof. B.V. Somov. ... 27 September 2013 The Solar Physics Department was visited by journalists of the leading Russian TV channel "Vesti-1". ...

... 00 30 50 20 40 00 30 00 30 00 30 30 Sunrise Registration of participants Opening of the conference and Memorial Coffee break Plenary session « i i i .. Group photo Lunch Section sessions Coffee break Section sessions Dinner Guitar concert Shevchenko memorial « » ( ) Sunset Welco me Party Tuesday, 19.08.2014 Sunrise Plenary session Coffee break Plenary session Lunch Section sessions Coffee break Section sessions Dinner : , " Sunset 20.03 21.00 ­ 23.00 06.00 09.30 ­ 11. 11.00 ­ 11. ...

Full-Text Search . ... arXiv.org . astro-ph . ... SAI VO . ... Whitespace-separated words are treated as AND ed. Show 10 50 100 articles per page in Full Compact mode . ... 1] oai:arXiv.org:astro-ph/9507093 [ pdf ] - 93031 . Beltrami Equation and Cluster Lensing: Characteristic Equations and Applications . ... Submitted: 1995-07-24 . Arclets in clusters of galaxies can be used to determine the lens mapping and not only to constrain the mass density of the cluster. ... SAI MSU . ...

В магнитосфере Земли обнаружены микровихри . 17 августа 2005 г . В 2000 г. Европейское космическое агентство отправило на околоземную орбиту квартет одинаковых спутников Cluster (все они имеют танцевальные названия - Salsa, Samba, Tango и Rumba). ... Тогда четверка спутников располагалась на орбите по углам воображаемого правильного тетраэдра, все стороны которого имели длину 100 км. ... Предыдущий документ - Следующий документ . ... Планета Земля . ...

... With the lithium line 6708 ° as a rough estimate for the stellar age, we show that the A "lithium" age of RZ Psc lies b etween the age of stars in the Pleiades (70 Myr) and the Orion (10 Myr) clusters. ... Thus, both estimates of the age of RZ Psc, based on the lithium excess and the proper motion of the star give values that essentially exceed the characteristic time of dissipation of protoplanetary disks ( 10 Myr; Strom, Edwards & Skrutskie (1993)). ... This source dominates in UX Ori stars. ...

NASA JOHNSON SPACE CENTER ORAL HISTORY PROJECT BIOGRAPHICAL DATA SHEET NAME: Thomas Patten Stafford O RAL H ISTORY: 15 October 1997 EDUCATIONAL BACKGROUND: BS with honors, United States Naval Academy, Annapolis, Maryland, 1952 Graduated from Squadron Officer School Graduated from Air Force Experimental Flight Test Pilot School, 1959 M ILITARY EXPERIENCE: Lieutenant General, United States Air Force , Retired November 1979 PRE- ... Transmitted first live color TV from space. ...

ARCSAT ID NUMBER: AS05 DESCRIPTIVE TITLE: Fundamental Properties of High Galactic Latitude Open Clusters PI: Ana Larson OBSERVER(S): Ana Larson, Joanne Hughes Clark UNCERTIFIED/UNTRAINED OBSERVERS:Daniel Larsen, Max Lutz COLLABORATORS: Joanne Hughes Clark CONTACT INFORMATION: dlarsen9@uw.edu 808-987-2176 lutzm@uw.edu 425-749-2812 jhughes@seattleu.edu anamunn@uw.edu TIME REQUESTED: ...

... AstroGuide | ... Astro Images . ... M45, Pleiades Cluster . Image by John Chumack, Galactic Images . M45 The Pleiades Cluster "The Seven Sisters." 45 minute exposure through 6: Takahashi Astrograph. Courtesy of John Chumack, Galactic Images . ... www.astronomy.net . About Astronomy Net | ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . are trademarks of John Huggins ...

... IAU planet classification Observing with a Telescope Large Scale Structure The observables: Local Group (size 1 Mpc) Virgo cluster (size 2+ Mpc) Virgo supercluster (size ~33 Mpc) Voids (size ~ 10-150 Mpc), Walls and sheets, aka filaments (size ~ 50-80+ Mpc) 1 parsec The nearest star is 1.2 parsecs away (Proxima Centuri). ... Virgo supercluster Voids, Sheets Filaments The Virgo Cluster is a cluster of galaxies at a distance of about 18.0 Mpc away in the constellation Virgo. ...

... Field of research: Extragalactic astronomy. ... NASA Astrophysics Data System (ADS) Abstract Service . ... CADC Home Page . ... CCD Images of Galaxies . ... RUSSIAN LINKS . ... UA Astronomy Personal Home Page - Bill Keel . ... The Shape of the Rotation Curves of Edge-on Galaxies, by A.V.Zasov and A.V.Khoperskov, 2003. ... A Thickness of Stellar Discs, by A.V.Zasov, and D.V.Bizyaev, 2003 . Minimum Velocity Dispersion in Stable Stellar Disks, by A.V.Khoperskov, A.V.Zasov, and N.V.Tyurina, 2003 . ...

... 0 ) = Z '' '' 0 [(1 \Gamma '')'' 1=2 sin 2 i sin 2!] ... We use the similarity theory to present the non--dimensional period T \ Lambda of the evolution of the parameters '' and i as a product of the independent factors: T \ Lambda = \ Gamma (4=15)(a \ Gamma3 =2 \ Lambda =LD )jL c (c 1 ; c 2 )j. Here LD = Ї k \ Lambda a \ Gamma3 k \ Lambda '' \ Gamma3 =2 k Ї \Gamma1=2 \ Lambda is the non-- dimensional parameter of disturbances similarity dependent on the dynamical characteristics of the ...

ASTEROIDAL DAMAGE TO THE EARTH: IMPLICATIONS BY ASTEROIDS ­ RUBBLE PILES. ... 13, Moscow 119892, Russia, E-mail:san@sai.msu.ru In the cause of asteroids ­ rubble piles its effective cross-section of collision to the Earth is determined not by consolidated body, but by cluster of its fragments. Since the stage of rubble ­ piles may be ~108 years (see our communication at previous symposium), it may be significant for estimation the asteroidal damage to the Earth. ...

It is the first scientific module included in OS. SPC Energy developed it. Module Kvant was launched on March 31, 1987 by LV Proton-K from the launching pad Baikonur. At the launch the module consisted of two docked units: module Kvant itself and transportation and energy module (after docking with the OS was separated and sank in the Pacific Ocean). ... The original mix of the scientific equipment was aimed at the astrophysics investigations. ...

. Welcome . Dmitriy Bizyaev d m b i z at s a i.m s u.s u .

N NGC N Созв. ... C-1 NGC 188 Cep OC Open cluster 00h 44.4m +85 20' 8.1 14 C-2 NGC 40 Cep PN Planetary nebula 00h 13.0m +72 32' 12.4 0.6 C-3 NGC 4236 Dra SG Spiral galaxy 12h 16.7m +69 28' 9.7 19 x 7 C-4 NGC 7023 Cep BN Bright nebula 21h 01.8m +68 12' -- 18 x 18 Refl. nebula C-5 IC 342 Cam SG Spiral galaxy 03h 46.8m +68 06' 9.2 18 x 17 C-6 NGC 6543 Dra PN Planetary nebula 17h 58.6m +66 38' 8.1 5.8 Cat's Eye Neb. ... C-103 NGC 2070 Dor BN Bright nebula 05h 38.7m -69 06' -- 40 x 25 Tarantula Neb. ...

... Левее Северной Короны расположено созвездие Геркулеса (лат. название Hercules, сокр. лат. ... Между Вегой и Геммой можно заметить четыре звезды Клина - астеризма, который представляет собой часть созвездия Геркулеса, руки и ноги которого "растут" из углов Клина . Между двумя западными звездами Клина - z и h Геркулеса - расположено шаровое скопление звезд М13 (Great Cluster), которое невооруженному глазу представляется туманным пятнышком 6 m , углового диаметра около 5'. ...