... From the chain visibility point of view, it is very recommended to look at the Javascript movies , especially if the frame rate can be not regulated in your MPEG player. ... The non-CH-associated large-scale chains visible on the SOHO/EIT images at three wavelengths of 171, 195 and 284 as well as on the MLSO/HAO He I 10830 spectroheliogram of December 16, 1997. ... The SOHO/EIT movies at 171 and 195 show the chain dynamics on June 1-3, 1998. ... Javascript movie (230 KB), SOHO/EIT, 171 . ...

. Last registration to attend . August 1 . Submission of abstracts (0.5p) . September 1 . Schedule of the Symposium . September 15 . The day of arrival . October 15 . Invited reviews and reports . October 16-19 . The day of departure . October 20 . Submission of contibutions (4pp) . November 1 .

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... We present simple stellar collapse physical model which allow us estimate the time evolution of the most important physical parameters of Black Holes --- mass and specific angular momentum and disk formation time. ... The disk accretion play important role in acceleration of BH rotaion. The BH specific angular momentum can reach value more than $0.9$ for wide range of stellar envelop angular momentum. Then with out disk accretion in case of power low stellar envelop it limited by value $0.45$. ...

... Registration form . ... Institute of Applied Astronomy of the Russian Academy of Sciences invites you to participate in the all-Russian scientific conference "Asteroid-Comet Hazard-2005" which will be held 3-7 October 2005 in St. Petersburg. ... Batrakov Yu.V. Institute of Applied Astronomy of RAS, St.Petersburg . ... Institute of Applied Astronomy of RAS . ... Finkelstein A.M. Institute of Applied Astronomy of RAS, St.Petersburg . ... Institute of Applied Astronomy of RAS, St.Petersburg . ...

Astronotes Armagh Planetarium's Stellar Blog! ... Many of the topics studied will have a local perspective, helping learners become better equipped to meet the needs of Northern IrelandтАЩs economy in an international context. ... Learners in the Space Science Technology qualification will build upon their existing skills in science, maths, engineering and ICT, and will use their new-found knowledge to solve real-life problems. ... Northern IrelandтАЩs New Space Science Technology Course | ...

. There may be security measures or other authentication procedures in use at your site that prevent you from using the rcp command to copy files from one host to another. Check with your local system administrator to find out what the situation is on your system.

... Our tours this year include: Yuri Gagarin Cosmonaut Training Center at Star City, Bauman Moscow State Technical University Orevo Laboratory, Russian Mission Control Center (TsUP), Rocket and Space Corporation Energia, Lavochkin Scientific and Industrial Association, Energomash Scientific and Industrial Association, Scientific and Industrial Association "Zvezda", Khrunichev State Research & Production Space Center, Monino Air Force Museum. Bauman Moscow State Technical University . Moscow) . ...

... LABORATORY OF RADIO ASTRONOMICAL OBSERVATIONS . Radio sources identification is one of the most important tasks of the current radio astrophysics. ... Optical idetification. ... Optical identifications of subsample of steep spectra radio sources from RC catalog using 6m SAO telescope of SAO RAS: optical observations. ... Astronomy Reports. ... Identification of radio sources with data of various radio catalogs allows one to construct continual spectrum of the object and its radio structure. ...

2013 ? ... Andrei Romashchenko (Laboratoire J.-V. Poncelet Moscow ? ... The Complexity year will extend the existing cooperation between the researchers from Moscow State University (Kolmogorov complexity seminar, Math Dept), Moscow Physics Technical University, Steklov institute, and researchers from LIAFA, LIRMM and other laboratories in France. ... Laurent Bienvenu visits Poncelet lab for the Complexity Year. He will teach a course (+seminar) on Kolmogorov Complexity and Computability. ...

... Tonight's Sky . ... Astronomy for Kids . ... Cosmic mirages" confirm accelerated cosmic expansion . ... The accelerated expansion increases the distance to the quasar, giving rise to higher chance of having a massive galaxy close to the light path to produce gravitational lensing. ... This research conducted an enormous survey of gravitationally lensed quasars and adopted much more sophisticated theoretical calculations to build a very convincing case for the accelerated cosmic expansion.т?? . ...

... Research objects and scientific purposes . Space scientific program includes development and launch of two supersmall spacecrafts "Universitetskiy" and "Kompas-2" intended for monitoring of radiation conditions near the Earth. ... All the studies conducted in the near-Earth space are characterised by strong radiation fields. ... The circular polar orbits, which cover all the near-Earth space, are the most favorable for comprehensive studies of the radiation conditions near the Earth. ...

... Telescopes ћ Binoculars ћ Microscopes . Meade Ultra-High Transmission coatings (UHTC ) Group . ... Meade Standard Coatings: The optical surfaces of all Meade telescopes include high-grade optical coatings fully consistent in quality with the precision of the optical surfaces themselves. ... These specialized, and extremely advantageous, coatings are offered here as the Meade Ultra-High Transmission Coatings (UHTC) group, a coatings group available optionally on many Meade telescope models. ...

... MAO main . ... IAU e-Newsletter - NameExoWorlds: An IAU Worldwide Contest to Name Exoplanets and their Host Stars . ... Тема: IAU e-Newsletter - NameExoWorlds: An IAU Worldwide Contest to Name Exoplanets and their Host Stars . ... Latest Press Release NameExoWorlds: An IAU Worldwide Contest to Name Exoplanets and their Host Stars . ... Welcome to the revamped version of the IAU e-Newsletter. ... IAU. ... NameExoWorlds: An IAU Worldwide Contest to Name Exoplanets and their Host Stars . ... MAO NASU ....

A 215 to 265 GHz spectral line survey of the Sgr B2 molecular cloud By A l b e r t Numme l i n e­mail: albert@bele.oso.chalmers.se Onsala Space Observatory, S­439 92 Onsala, SWEDEN The spectrum of the Sgr B2 molecular cloud has been surveyed between 215 and 265 GHz towards 3 positions, the dense cores Sgr B2(N)and Sgr B2(M), and the quiescent core Sgr B2(NW). ... 1993)). ... 1991)). ... Albert Nummelin: Spectral line survey of the Sgr B2 molecular cloud 3 Lis D.C., Goldsmith P.F., 1991, ApJ, 369, 157. ...

... The following changes have been initiated by user feedback: . ... SAOtng command line options can be stored as csh-style environment variables in the ~/.saotng file. ... See SAOtng Command Line Options for more information. ... See SAOtng Colormap Considerations for more information. ... We have added the ability for SAOtng to resize image frame #1 each time a new image is loaded (as did SAOimage). ... See Autoflip of Images for more information. ... See Marker Analysis in SAOtng for more...

... Form of the Latitude Distribution of Sunspot Activity V. G. Ivanov* , E. V. Miletskii, and Yu. ... It is shown that the latitude distributions of sunspots for a given year can be approximately described by the normal law, with its variance being a linear function of the current level of solar activity. ... However, the latitude distribution of sunspots and its dependence on the activity level remained unclear. ... 55 No. 10 2011 the relative sunspot distribution for each range (see Fig. ...

Pulsar - the neutrone star. ... Its physical properties are greatly changed. ... Naturally after the discovery of pulsar connection with the remains of the supernew star outbursts it was supposed that the pulsars and the neutron stars are the same objects. ... In the external layer of a neutron star, where the substance dense is not so great to break the cores; they may from the hard chip structure, which at the pulsar rotation decreasing is broken the starquake. ...

Static Fourier spectrometers are often used for spectral measurements of the ionosphere emissions. There are two main advantages of Fourier spectrometers (FS) - large geometric factor and high spectral resolution; these parameters are two orders better than for grating spectral instruments. ... In scanning Fourier spectrometer optical and electric modulation of signal is used to avoid this problem, for static Fourier spectrometer there are no such ways. ...