... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... ISS Russian Segment . ... Build an operational model of neutron background environment on the station; . ... Correlation data on radiation environment parameters outside the Service Module of the ISS RS obtained through calculation with the results of measurements made by science hardware BTN-M1 and results of other Russian and international experiments; . ... 2015 JSC "S.P. Korolev RSC "Energia" ...

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• INTERNATIONAL SPACE STATION

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Investigations of the ionospheric response to strong magnetics storms which are usual for our latitudes, are of great interest. ... In the figure, we present ionospheric parameter dynamics during three perturbed days in July 2000. ...

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• East Siberian Center for the Earth's Ionosphere Research. Capabilities and

... Mokhovaya st., 11, Moscow, 103907, Russia. ... Proceedings of the 6th IEEE International Specialist Workshop on Nonlinear Dynamics of Electronic Systems, Budapest, Hungary, 16-18 July, 1998 , pp. ... The method for synchronization of drive-response systems on conditions of a large mismatch of parameters is considered on example of the system based on modified Chua's circuit. The approach to information transmission using such method is proposed. ...

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• Project 1 - SfP - Ovsyannikov, Supersensitive high-Tc superconducting

... Number of above the background required for a detection (this parameter is passed to omdetect , see the description of omdetect . ... Half-width of the spectrum extraction region (in pixels, if negative, and in FWHWs otherwise) . ... Offset of the left background extraction region from the edge of the spectrum extraction area; in pixels, if negative, or in FWHWs otherwise. bkgwidthleft . ... Width of the left background extraction region; in pixels, if negative, or in FWHWs otherwise. bkgoffsetright...

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... Polar Cap Potential . ... The solar wind propagation delay time calculation used here is conceptually similar to the T(IMF) calculation in Kelly, et al. ... The older continuous data are from key parameter data files. ... Note: Very high values of Solar Wind Speed, Solar Wind Pressure, IMF Magnitude and Bz, and Polar Cap Potential are likely indications that WIND has reentered the Earth's magnetosphere; such data is not indicative of solar wind conditions or impending severe geomagnetic disruption. ...

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• List of currently available KP AZ.
• ENERGETIC PARTICLE EXPERIMENT DOK-2
• ASPI experiment

... Obviously, the size of the cavern is of the order of the Schwartzman radius. ... Thus, consideration of the inverse effect of pulsar radiation on the properties of accreting plasma makes the ejection possible even when the Schwartzman radius is smaller than the capture radius. ... If the cavern radius , the condition at its boundary can be written as . ... Apart from magnetic dipole radiation, the cavern may also contain relativistic particles (which are also reflected from the cavern boundary). ...

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• Other parameters of the evolutionary scenario
• Dependence on the Scenario Parameters and Initial Distributions
• The Gravimagnetic Parameter

... and prior, see paper files. ... OREXP 05-02) E. Torrence, "SR Energy Spectrometer" , Machine-Detector Interface at the International Linear ColliderWorkshop, January, 2005. ... OREXP 05-05) J. Brau, "The International Linear Collider: Physics, Detectors, the Accelerator, and the Roadmap" , Seminar, UCLA, Febuary, 2005. ... OREXP 05-25) E. Torrence, "Energy and Luminosity Spectrum" , 2005 International Linear Collider Physics and Detector Workshop and Second ILC Accelerator Workshop , August, 2005. ...

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• University of Oregon Center for High Energy Physics - Recent Experimental Talks
• U of O Experimental High Energy Physics
• Potential Energy

... Research of an atmosphere of the Earth and other planets of Solar system by optical methods . ... The long-term experience of study of atmospheres of planets of Solar system in a department of physics of planets has defined directions and methods of researches spent for laboratory . ... The tasks of laboratory are researches by optical methods of structure of a Terrestrial atmosphere, namely study of spectra of absorption of its compound radiation of natural and artificial sources. ...

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• Activity - Page 2
• Aspherical optics
• Publications

Stationary Shock Waves. ... Influence of Medium Ionization on Shock Wave Propagation. Shock Waves with Decays. ... Results of Classic Theory of Radiation of the Electron Moving in Ion Field. ... Classification and Physical Features of Galaxies. X-Radiation of Coronae of Elliptical Galaxies and Clusters of Galaxies. ... Methods of Obtaining of Information about Physical Conditions and Components of Interstellar Medium. ... Ionization Fronts and Shock Waves in the Interstellar Medium. ...

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• Theoretical Astrophysics
• ENERGOSPECTROMETER OF IONOSPHERIC PLASMA P3-3
• Solar Physics

... Tte tables of ionosphere and plasmasphere parameters are contained in a file param.tbl. ... Latitude Longitude Numbers of tables for (degree) (degree) Month Wm=10 Wm=100 Wm= 150 80 30 March 1 - 3 397-399 793-795 80 150 March 4 - 6 400-402 796-798 80 270 March 7 - 9 403-405 799-801 60 30 March 10 - 12 406-408 802-804 60 150 March 13 - 15 409-411 805-807 60 270 March 16 - 18 412-414 808-810 40 30 March 19 - 21 415-417 811-813 40 150 March 22 - 24 418-420 814-816 40 270 ...

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• http://www.wdcb.ru/stp/data/mod_I_P/DRAFT.TXT
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/M3000
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/F

Russian version] . ... Collective phenomena in dusty plasmas under laboratory and microgravity conditions " . ... Effective structural (pair correlation function) and transport (diffusion constant, formation of dust vortices) characteristics of the system of microparticles (dusty plasma) have been measured in a set of experiments in dc- and rf gas-discharge plasmas in ground-based and microgravity conditions on the board of Russian ''Mir'' Space Station and International Space Station. ...

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• Space experiment "OBSTANOVKA 1-st stage"
• PLASMA EXPERIMENTS ON TAIL PROBE
• Космический эксперимент "ОБСТАНОВКА 1-й этап"

... Research . Projects . ... The name of the project APEX is a reduction from words " Active Plasma Experiments " . The core of the project are active experiments with injection of electron and (or) plasma beams from a board of the satellite with simultaneous registration of the phenomena, produced by interaction of injected beam with background plasma. ... Active experiments utilise modulated electron beam accelerator and source of modulated xenon plasma beam on the main spacecraft APEX. ...

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• Ionospheric plasma-wave interaction
• History

Next: A New IRAF Catalog Access Tool for Astrometry . Up: Iraf Packages . ... Twofitlines is a tool developed within IRAF, optimized to be used with data containing multiple spectra along the spatial axis of the detector. A given spectral feature can be decomposed in one or several Gaussian components. ... A given spectral feature can be modeled using one or more components (currently only Gaussian profiles are available), . ... Close spectral features could be modeled simultaneously. ...

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• A New Entropy Measure Based on Multiple Resolution and Noise Modeling
• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
• VLT Data Quality Control

The central velocity dispersion represents the internal motions of the stars along a column crossing the center of a galaxy or star cluster. ... The catalogue of collected velocity dispersions may be accessed in HyperLeda. vdis is the velocity dispersion given in km/s. The velocity dispersion gives to some approximation the scale for the specific kinetic energy contained in in un-ordered motions and combined with the velocity of rotation it may give an estimate of the specific kinetic energy. ...

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• Line parameter measurements
• Outline of the Available Methods
• HyperLEDA documentation: parameter: celpos

... Luminosity (L) · · · · A source's luminosity is the power that it emits in radiation. ... NB Astronomers often say `flux' when they mean `flux density' · SI units are Wm-2Hz -1 -26 filter · Also used are Jy 10 Wm-2Hz -1 E= РРРF d dA dt Specific Intensity, Surface Brightness (I) · Specific intensity (or surface brightness) is the power received (or emitted) per unit area per unit frequency per unit solid angle. ч F at surface of a spherical source = I · · Specific intensity is independent of distance...

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• ALMA Phase Calibration Techniques at the Cavendish Astrophysics Group
• PPEUC Programme - Cosmic Microwave Background Workshop
• DUST: dustiface.h File Reference

... RSC Energy General Designer . ... The possibility of continuing the exploitation of the complex in the conditions of the inevitable obsolescence and depreciation of the on-board equipment providing the achievement of the necessary level of safety has been one of the most important and always controlled problems during all the term of exploitation of the complex Mir. ... The technical condition of the complex Mir gives the opportunity to continue its exploitation in a piloted mode till 2002 and more....

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• RAS ISR' Conclusion on the scientific results received in the orbital complex
• The project of the joint international exploitation of the piloted space

New reduction of minor planets photographic plates obtained with Pulkovo Normal Astrograph A.A. Berezhnoy Pulkovo Observatory of RAS, Saint-Petersburg, Russia Minor Planet observations at Pulkovo Periodical observations of 14 bright asteroids named Selected Minor Planets (SMP) were performed at Pulkovo since 1948 within the international framework started by works of B.V. Numerov and D. Brouwer. ... 108 133 113 74 124 67 97 88 14 84 64 5 20 19 Epochs (YYYY.MM) 1200 Mean values of total obs. ...

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National Research Institute for Physical-Technical and Radio Engineering Measurements IMPROVEMENT OF THE SOFTWARE BERNESE FOR CALCULATION OF THE EARTH ROTATION PARAMETERS ACCORDING TO THE DATA OF SATELLITE LASER RANGING (LAGEOS 1, LAGEOS 2) IN THE MAIN METROLOGICAL CENTRE OF THE STATE TIME AND FREQUENCY SERVICE Tsyba E. N., Kaufman M. B. 141570, Mendeleevo, Moscow region, Russia tel. +7-903-194-7575; tsyba_e_n@mail.ru ABSTRACT Preparatory ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/suvorkin.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm12i.pdf
• http://www.gao.spb.ru/russian/psas/ffk2013/tfiles/yerokhin_H2_FFK13.pdf

2.1 Ramp filters (ACS, WFPC2) . ... 2.4 Encircled energy (ACS, WFC3) . ... 2.4.3 Supported ACS Aperture Sizes . ... Parameterized keywords are generally used to access throughput tables for which the throughput is a function of some other variable in addition to wavelength. The syntax for a parameterized keyword is keyword#value , where value is a numeric (integer or float) value for the keyword to take. ... If no parameterized keyword is used in the obsmode, a default value will be used. ...

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• How precise are the parameters of my double star as measured in Transfer Mode?
• Fundamental Parameters, Integrated Red Giant Branch Mass Loss, and Dust
• Index

... Science User Portal . ... ESO, the European Southern Observatory . ... Travel and Contacts . Travel to ESO Headquarters . ... Travel to E-ELT Armazones . ... ESO Acronyms . ... Survey Telescopes . ... Star Clusters . ... Stars@ESO . ... Catch a Star 2013 . ... The dark red region for the galaxy cluster determination corresponds to 95% certainty (2-sigma statistical deviation) when assuming good knowledge of all other cosmological parameters, and the light red region assumes a minimum knowledge. ...

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• Constraining the Cosmological Parameters | ESO United States
• Constraining the Cosmological Parameters | ESO Ireland
• Constraining the Cosmological Parameters | ESO Australia