... STScI previously used Microsoft Word and Microsoft Access, a Sybase ODBC driver, and the Adobe Acrobat PDF writer, along with a substantial amount of Visual Basic, to generate a variety of documents for the internal Space Telescope Grants Administration System (STGMS). ... To create a document, the internal STGMS application invoked a VB program which launched Microsoft Word and Microsoft Access, Access extracted the required data from a Sybase database using ODBC into an Access table. ...

Добро пожаловать, Гость . ... Горизонты науки о Вселенной (Модераторы: Дмитрий Вибе , AlAn ) ? Торсионные поля . ... 0 Пользователей и 1 Гость просматривают эту тему. Гость . Ответ #180 : 10.08.2006 [21:47:48] ? Цитата: Rangelov от 10.08.2006 [14:15:45] Извини9е, однако я не понимаю, как можно возбуждаь спин, если не вбуждения, ко9орое кру9и9ся? ... Ответ #181 : 15.08.2006 [08:07:02] ? ... Ответ #182 : 16.08.2006 [12:38:23] ? ... Ответ #183 : 16.08.2006 [15:52:45] ? ...

... Right: cold gas traced by [CII] emission (red) accreting onto a primeval galaxy (green) at z=7.1 ( Maiolino et al. 2015 ) (image credit: ALMA Press Release ) . ... 2010 , Cicone, Maiolino et al. ... 2012 , Cicone, Maiolino et al. ... Right: observed distribution of the average stellar metallicities of passive and star forming galaxies in the local universe, supporting starvation/strangulation as primary quenching mechanism in low/intermediate mass galaxies ( Peng, Maiolino, Cochrane 2015 ). ...

... The remote area was formed very early, at a time when the Universe was a fifth of its present age and the presence of the galaxy string defies existing models, which can not explain how a string this big could have formed so long ago. ... The simulations tell us that you cannot take the matter in the early Universe and line it up in strings this large," Dr Francis said. ... But in the early Universe, most galaxies had not yet formed, and most dark matter clouds will not yet contain a galaxy. ...

... Observing may be done from any location. ... See this link for further details, limiting magnitude charts, and star count tables: http://www.imo.net/visual/major/observation/lm Proof Point Information : Shapley-Sawyer Classification: Reference: http://x.astrogeek.org/articles/article.php?article_id=15 Brief Description: I - High concentration toward the center; E.g ., NGC 6864, M75 II - Dense central condensation; E.g ., NGC 7089, M2 III - Strong inner core of stars ; E.g ., ...

V. Barale, Joint Research Centre, European Commission, Ispra, Italy; M. Gade, University of Hamburg, Germany (Eds.) Remote Sensing of the European Seas Here is a review of the current potential of Earth Observations that devotes particular attention to the challenges posed by the European Seas. ... Part 1: Introduction.- ... Pre-publication pricing: Unless otherwise stated, pre-pub prices are valid through the end of the third month following publication, and therefore are subject to change. ...

U.S . Astronomy Facilities For the 21st Century Bob Dickman National Science Foundation Building the Foundation for U.S . Astronomy at m/cm Wavelengths in 2010 and Beyond This foundation will require money Ground-based radio astronomy has historically relied on NSF funding It may be useful to point out some of the challenges which all new NSF astronomy ... Cost -- $nB/3 (FY06) must have n<2 Engineer the instrument -- it is not too soon Optimize US organization Goals Representation ...

Общий форум . Scientific.ru Все форумы . Постоянные участники форумов [ .. ... илья исаевич элиович доктор техн. наук профессор (@) - 09.06.2005 09:27 . information in brain power processing . NEW INFORMATION TECHNOLOGY - Authoring User's Languages. ... Одновременно это является и тем, что входит в сферу представлений Brain power processing. [ прямые ответы (1) ] . ... information in brain power processing илья исаевич элиович доктор техн. наук профессор, 09.06.2005 09:27 . ...

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Partners in Learning: a 12-minute videotape from Project ASTRO funded by NASA's Office of Space Science . How does Project ASTRO work? ... Listen to project participants share the rewards of their efforts and see students' enthusiasm for learning about science in Project ASTRO classrooms. This video is available as part of the Universe at Your Fingertips 2.0 DVD-ROM. 390 Ashton Avenue, San Francisco, CA 94112 . ...

Russian version] . ... Future seminars . P a s t seminars . ... 2010 - 200 9 . 200 8 - 200 7 . 200 6 - 2005 . ... Seminar council . PAST SEMINARS (2012) . ... O.G. Bakunin (Kurchatov Institute) . ... A.V. Milovanov (Space Research Institute, ENEA ) . ... D.O. Chernyshov and V.A. Dogiel (P.N.Lebedev Institute of Physics) . ... A.V. Byalko ( L.D. Landau Institute for Theoretical Physics, Russian Academy of Sciences, Chernogolovka, Moscow region, Russian Federation ; Journal 'Priroda' ) . ...

Computers become more and more popular nowadays. That means that the amount of people who are able to work with computer programmes and play computer games has increased. In many cases computer games are the only thing that a person is accustomed to. ... As a result of this epidemic "homo playing" may put on the isoreality helmet which makes a person, crazy about games, forget about food, slumber and all other components of real life: "homo playing" becomes isolated from community. ...

... Programme . ... Non-equilibrium dynamics and radial migration in the disc . ... Introduction to orbit-superposition models. How do we fit such a model to a catalogue? ... Torus modelling as an extension of Schwarzschild; respects in which it supercedes Schwarzschild . ... In what detail can we represent the MW in a conventional N-body model? ... Given the Gaia catalogue, an NIR catalogue (VHS?) and a dynamical model, how to build a dust model? ... How to optimise complex models? ...

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... ,E_=v_B_z,B_z0 Light cylinder at RL U = electric voltage created by rotating BH I = large scale current I U LK Centrifugal acceleration in BH magnetosphere Assume `reasonable' B and E fields, from current I : Bz = 0 = v/v 1 Motion of a test particle P ( ) Light cylinder Pz() P() z() Here = 0.01 and = rc,i/RL = 0.01 Growth of particle Lorentz factor ( ) log k At light cylinder : = Here with initial value is the absolute maximal reachable by this process (ie no ...

... 8, ``Celestial Mechanics'', 2002 Two problems in solar systems dynamics, possible solutions and future A. Fienga IMCCE­Observatoire de Paris, Paris, France In this contribution, two major aspects of the new challenges of the solar system dynamics are presented. ... As it was demonstrated by (Standish and Fienga [4]), the perturbations of the Mars orbit by the asteroids are difficult to modelize and they present now the main limitation of the present theory of Mars motion. ...

After some period of quiet Sun the exciting Sun-Earth connections event as the big magnetic storm was observed at January 10-11, 1997 by various satellites and ground-based instruments. Scientist meet this challenge with unprecedented activity and a few data bases was created in relation with solar event/magnetic storm on a few WEB-sites. ... According the Moscow observatory data the sudden storm commencement (SSC) take place at 01:08 Universal Time of January 10, 1997. ...

Summary of the research statement My research pro ject is dedicated to motives and cohomology theories; its main sub ject areas are algebraic geometry and homological algebras, yet certain relations with number theory and algebraic topology could possibly be studied. ... One of the open problems for the theory of motives was the introduction of certain 'weights' for them; it was solved by the applicant in quite a satisfactory (though rather unexpected) way. ...

... Phil Creed's Astronomy Bowl! ... Hidden Hollow's Astronomy Bowl is a fast-paced question-and-answer game designed to both enlighten and challenge stargazers. ... Astronomy Bowl follows the traditional format of alternating toss-up and bonus questions, with a few tweaks. ... The host will read a toss-up question. ... Once a toss-up is correctly answered, that team is given a bonus question. ... If only 14 toss-ups are answered correctly, that means 20 toss-ups and 14 bonus questions will be read. ...

Discussion Forum Calibration Targets -------------------------------------------- Keith Jahoda sumarised the'Cal targets' group. Group generated a list of CAL targets, with their uses. ... Energy scale and line width at high energies, especially for Con-X. No obvious celestial targets. ... Not easy to cover 0.1->100 keV. ... RM - temp profile of cluster problem. XMM and Chandra give different answers - Chandra give higher temp by upto 1.5 keV for hig htemp clusters. ...