... Pustilnik S.A., Ugryumov A.V., Lipovetsky V.A., 1993, Clustering of voids as an appearance of super-large scale structures. in Proceeding of Int. Workshop on Galaxy clustering and large-scale structures in the Universe" . ... Pustilnik S.A., Ugryumov A.V., Lipovetsky V.A., Thuan T.X., & Salzer J.J.: Large-scale spatial distribution of BCGs from the new large samples -- Byurakan and Case surveys. in Proceeding of ESO/OHP Workshop Dwarf Galaxies" , 1994, p.133-136. ...

... LP-Moon.pdf - 26KB . ... A. A. Berezhnoy1,2, N. Hasebe1, M. Kobayashi1, G. Michael3 and N. Yamashita1 1Advanced Research Institute for Science and Engineering, Waseda University, Tokyo, Japan 2Sternberg Astronomical Institute, Moscow, Russia 3German Aerospace Center, Institute for planetary research, Berlin, Germany . Brown University - Vernadsky Institute Microsymposium 40, 2004, Moscow, Russia . ... 3Now at: Sternberg Astronomical Institute, Moscow University, Moscow, Russia . ...

Обзоры hep-ex: тематический рубрикатор . ... hep-ex/0306011 . Рождение векторных мезонов и инклюзивного канала K s K s на HERA . ... Authors: M. Barbi (McGill University), for the H1 Collaboration, ZEUS Collaboration . Comment: 6 pages, 6 figures, to appear in the proceedings of the International Conference on the Structure and Interactions of the Photon, Frascati (Italy), 7-11 April 2003 . ... Comments: 9 pages 5 figures submitted to PRL . ... Comments: 13 pages, 1 table and 4 figures . ...

Next: Data Acquisition with Up: Data Acquisition Previous: Data Acquisition . The main method of finding targets is a modified version of the classical star hopping method. ... General preparation would include several finder charts; a wide constellation field, the 30mm field, the 3" field and the of the 14" field. ... The 30mm has a field of view of 2.5 arcminutes, the 3" has a 40 arcsecond field of view; each camera's field of view is specified in Table 1. ...

... Partly based on observations performed with radio telescopes of IAA RAS (Federal State Budget Scientific Organization Institue of Applied Astronomy of Russian Academy of Sciences). c . ... Partly based on observations with the 100-m telescope of the MPIfR (Max-Planck-Institute for Radio Astronomy) at Effelsberg . ... NRAO facilities . The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. ...

NASA JOHNSON SPACE CENTER ORAL HISTORY PROJECT BIOGRAPHICAL DATA SHEET NAME: Robert O. Piland O RAL H ISTORY: 21 August 1998 EDUCATIONAL BACKGROUND: B.S. in Mathematics, College of William and Mary, Williamsburg, Virginia ... in Organization, University of Colorado at Denver, Denver, Colorado, 1984 M ILITARY EXP April 1947) ERIENCE: Aviation Cadet, V-5 Program , United States Navy (July 1945- PRE- ... New York: American Institute of Aeronautics and Astronautics, 1977. ...

Authors: Yu.G. Shevelev , V.A. Marsakov , . ... We have constructed and investigated properties of metallicity function of disk stars with different ages, proceeding from the statistically restored real altitude distributions of stars at the solar galactocentric distance. It is shown that the metallicity distribution of stars in each age range is not of Gaussian form, but it may be considered as a superposition of two normal distributions centered at -0.2 and 0.0 dex. ...

MATHEMATICAL MODELING: . ... This model is developed on the base of the probabilistic description of the collisional aeronomical processes and is realized on a computer as the numerical system (stochastic model). ... Shematovich, V.I., Bisikalo , D.V.             Nonequilibrium processes in the planetary and cometary atmospheres. ... In Russian) . ... Piarnpuu , A. A.; and Shematovich, V. I.       Construction of structural stochastic models of collision processes in rarefied gas media (abstract) . ...

... It is found that the correlation coefficients between these two parameters calculated separately inside and outside the sunspot formation zone ±30 have cyclic variation and occur in anti-phase. This suggests different mechanisms of formation of the corona in the fields of small, medium, and large scales. ... The relationship between the coronal green line brightness (CGLB) and the magnetic field strength (MFS) has been investigated by constructing the corresponding synoptic maps for the 1977-2001. ...

...you are entering the Mir's docking module... A glance back on the same hatchway from inside.....and you proceed towards the Kristall module .