p The 6th INTEGRAL workshop i ``The Obscured Universe'' /i will take place at the a href = http ://arc. iki .rssi.ru/ eng /index.htm Space Research Institute ( IKI ) /a , Moscow, Russia on July 2-8, 2006 (the working days July 3-7). /p p The main goal of this workshop is to consider (via invited and contributed talks and posters) the scientific problems in the field of high ... For you convenience cash mashine is located inside IKI building.</i> ...

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• Истомин Яков Николаевич (ФИАН)
• The 6th INTEGRAL Workshop "The Obscured Universe"

The Python programs offered here result from the development of methodology for processing image data with high precision, in a flexible command line system useful for astronomical and laboratory image processing. ... Alsvid is efficient in robotic and automated or scripted server processing of astronomical images, and also in interactive command line processing for research and visualization. ... In large part it replaces IRAF and IDL when scripted image processing is required. ...

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• FHT (ImageJ API)

Abstract -- Calculations are performed for the linear polarization of starlight due to extinction by aligned dust grains when the starlight traverses a medium with irregular magnetic fields. This medium is intended to represent the optically thick components of interstellar clouds which are observed to make little, if any, contribution to the polarization of starlight. ...

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... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... Brief History of Rocket and Space Technology . ... Flights Chronology . ... ISS Russian Segment . ... History of flights . ... History of Manned Flights | ... The MIR Station has become a peculiar flight site for real-time validation of many technical solutions and production processes used on the International Space Station. ... Contribution of RSC Energia to the Russian Rocket-Space Technology ....

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• S.P. Korolev RSC Energia - International Space Station
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... 18941904; Bespalov P.A. Effective saturation of absorption in a plasma magnetospheric maser. In book: Nonlinear Space Plasma Physics, R.Z. Sagdeev -Editor-in-Chief, American Institute of Physics, 1993, p.339-346]. Magnetospheric plasma maser [Bespalov P.A, Trakhtengerts V.Yu., ... In a magnetospheric plasma maser (MPM) the relatively dense magnetised plasma and the conjugate ends of a magnetic trap form a quasioptical resonator for electromagnetic waves. ...

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... ASRAS Board Members . ... Site . ... ASRAS Board Positions . ... President - . ... The president has many responsibilities like running monthly meetings, running the monthly board meeting, representing ASRAS at local events like star parties, planetarium events, RMSC events, the monthly newsletter presidents message, etc .. ... The Vice Presidents position is mainly to assist the president and back them up if they cant make a major function like a general meeting or write the newsletter pres message...

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• THE BRIGHT SUPERNOVA 1991T IN NGC 4527; AN AMATEURS PRESPECTIVE

... The defining location and structure of airglow needs tomographic processing of data of photometric measurements. ... Both observed function of column brightness and volume emission rate function of airglow may be expanded in a Fourier series. ... There are developed software and made numerical simulation for tomographic data processing. ... In this case airglow has gaussian profiles on both coordinates altitude and latitude. ... Total number of simulated observations is 320. Fig. ...

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• Publications of Astronomy and Space Physics Department
• Mykola I. Dzubenko
• WARNING MISSION: Background

... 4.4 Imbedding HTML in a Document . In the following discussion of SPECIAL processing
, I will assume that rtftohtml has not been customized. If it has, the text styles used to create special effects may be different. ... Normally, if your RTF document contained the text "<cite>hello</cite>", the translator would output this as: "&lt;cite&gt;hello&lt;/cite&gt;". ... If, however, you want the <cite></cite> to be interpreted as HTML markup, you must format the tags using Hidden and Shadow. ...

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• Killing processes
• Suspending a foreground process
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Solar Eruptive Event of 4 November 2001 observed with the SPIRIT Telescope on Board the CORONAS-F Satellite . ... Based on the data of the SPIRIT telescope on board the CORONAS-F satellite in three EUV channels 175, 284, 304 , we have analyzed large-scale manifestations of the post-eruptive so-lar activity followed one of the most considerable and geoeffective coronal mass ejection (CME) in the 23rd cycle which occurred on 4 November 2001. ... Posteruptive arcade on the CORONAS-F/SPIRIT movies at . ...

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• CMEs and Space Weather

... 8, ``Celestial Mechanics'', 2002 Two problems in solar systems dynamics, possible solutions and future A. Fienga IMCCEґObservatoire 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. ...

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RADIO EMISSION OF THE MOON BEFORE AND AFTER THE LUNAR PROSPECTOR IMPACT Berezhnoi A.A.*, Gusev S.G.**, Khavroshkin O.B.***, Poperechenko B.A.**, Shevchenko V.V.*, Tzyplakov V.A.*** * Sternberg Astronomical Institute, Universitetskij pr., ... For the registration of lunar RSR after the Lunar Prospector impact radio observations of the Moon on the two 64-m radio telescopes of the SDO MEI at Medvezh'i Ozera and Kaliazin were conducted during July 30 - August 2, 1999. ...

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Space-VLBI with RadioAstron : new correlator capabilities at MPIfR PoS(EVN 2014 )119 G. Bruni1 , J. M. Anderson1,2 , W. Alef1 , A. Lobanov1,3 , J. A. Zensus1 1 2 Max-Planck-Institut fЭr Radioastronomie, Auf dem ... Potsdam, Germany 3 Institut fЭr Experimentalphysik, UniversitДt Hamburg, Luruper Chaussee 149, 22761 Hamburg, Germany E-mail: bruni@ mpifr -bonn.mpg.de DiFX is a correlator for VLBI ... This enables the RadioAstron data to be converted into a format supported by DiFX. ...

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... October Monthly Meeting - Amateur Contributions in the Era of Surveys . ... Thursday, Oct 9, 2008 at 8:00 PM . ... Commercial CCDs and telescopes make this possible at modest cost for bright objects, and large, wide field professionalsystems like PanSTARRS and LSST extend coverage to fainter magnitudes. ... Please join us for a pre-meeting dinner discussion at Changsho, 1712 Mass Ave, Cambridge, MA at 6:00pm before the meeting. ... Oct . ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

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• Amateur Telescope Makers of Boston ATMoB Observing Awards Program

Solar Phys (2012) 276:97ґ112 DOI 10.1007/s11207-011-9883-6 Investigation of Hot X-Ray Points ( HXPs ) Using Spectroheliograph Mg XII Experiment Data from CORONAS-F/SPIRIT A. Reva Ї S. Shestov Ї S. Bogachev Ї S. Kuzin Received: 10 May 2011 / Accepted: 18 October 2011 / Published online: 24 November 2011 ? Springer Science+Business Media B.V. 2011 Abstract Observations in the Mg XII 8.42 е line onboard the CORONAS-F satellite have revealed compact high ... Figure 7 Intensity variation of HXPs. ...

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THE STUDY OF THE PIONEER ANOMALY THE STUDY OF THE PIONEER ANOMALY The Pioneer Anomaly : Effect, New Data and New Investigation Slava G. Turyshev Jet Propulsion Laboratory, California Institute of Technology Seminar at the Sternberg Astronomical Institute Moscow State University, Moscow, 6 February 2007 1 THE STUDY OF THE PIONEER ANOMALY THE STUDY OF THE PIONEER ... Are they relevant to the Pioneer anomaly? ...

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Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Although their determination is based on the scattering process model, independent check-ups by rocket experiments have shown their correctness in experimental applications. ... Ionospheric data analysis, especially during strong disturbances, cannot be without some other kinds of diagnostic tools. ... The lack of data has always been a challange in this case. ...

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... 329, P L41-L44 (1998). Abstract . ... 329, P L45-L48 (1998). ... 329, P L49-L52 (1998). ... 329, P L53-L56 (1998). ... 329, P L57-L60 (1998). ... 329, P L61-L63 (1998). ... 329, P 799-808 (1998). ... 329, P 809-820 (1998). ... 329, P 821-826 (1998). ... 329, P 827-839 (1998). ... 329, P 840-844 (1998). ... 329, P 845-852 (1998). ... 329, P 853-862 (1998). ... 329, P 863-872 (1998). ... 329, P 873-894 (1998). ... 329, P 895-905 (1998). ... 329, P 906-910 (1998). ... helpdesk@link.springer.de ...

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• Springer LINK:A&A-EE: Table of Contents Volume 330 Number 2 (1998)
• Springer LINK:A&A-EE: Table of Contents Volume 323 Number 1 (1997)
• Springer LINK:A&A-EE: Table of Contents Volume 332 Number 2 (1998)

... Публикации: "Odessa Astronomical Publications", 1997, vol. ... There are four basic forms (REGISTRATION, HOTEL RESERVATION, PAPER % CONTRIBUTION and PAYMENT) to be completed and returned to the CONTACT % ADDRESS mentioned below. ... SUMMER SCHOOL 10 Dundee Remote Sensing Summer School 49 Scottish Universities Summer School in Physics Physical Processes in the Coastal Zone: Computer Modelling and Remote Sensing 12th August to 29th August 1997. ...

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... Pre-assembly and testing of the echelle goes on in the 2.5m work area and on the intermediate level of the 3.5m. Jeff Sundwall/UC has arrived to contribute to the effort. He lends his expertise and light touch making adjustments to the camera. ... While Jeff moves on to work on the front end of the camera. The work being done on the observing level has been moved back downstairs. ... Shui and Connie are putting the optics into the tank this weekend. The tank should be mounted on Monday. ...

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• ARC 3.5m | TRIPLESPEC
• Astrophysical Research Consortium - Apache Point Observatory
• Untitled Document

... Spherical aberration, coma, and astigmatism are also easily observed using the star test. ... Off-axis images are complex. ... Fig. ... Diffraction by a circular aperture as a function of defocus for no aberration Airy Disk 1 wave defocus Less than 1 wave defocus Fig. ... Diffraction by a circular aperture as a function of defocus for third-order spherical aberration Paraxial Focus Small distance inside paraxial focus Moderate distance from marginal focus Immediate neighborhood of marginal focus Fig...

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• http://vega.inp.nsk.su/~inest/astrolib/Sun/kursoviki/Model2000/AtmModel/UV/README
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