... Future seminars . ... Within the framework of the " Space weather " program, 25-year sets of observations of solar x-ray radiation, measurements of parameters of plasma and a magnetic field in the solar wind and variations of Dst index are analyzed with the purpose of revealing the factors rendering the greatest influence on development magnetospheric storms. ... The data on the other type of solar activity - coronal mass ejection (СМЕ) - cover only small part of a researched interval. ...

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• Институт космических исследований РАН (ИКИ РАН)
• Main results of the experimental and theoretical research completed in 2009

Databases (NSDC) of the Natural Planetary Satellites. ... NSDC: Database of astrometric observations of Natural Planetary Satellites . ... They are thoroughly looking for observations in different sources, creating their owndatabases which are then mostly inaccessible to other researchers. ... In the file "content" with explications, the reference is given to the data source as well as the bibliographic reference. ... Data sources. ... Why a specific bibliographic database for Natural satellites? ...

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• Scientific activity
• Maidanak Lab page

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. Modelling, secondary
• East Siberian Center for the Earth's Ionosphere Research. Capabilities and
• East Siberian Center for the Earth's Ionosphere Research. Specific character

Atmospheric influence on the different radio-engineering system functioning . ESTIMATION OF ATMOSPHERIC OPTICAL CHARACTERISTICS AND REMOTELY SANSED IMAGE CORRECTION . ... Direct transmittance estimation results for 12 channels of the spectrometer CHRIS. ... We have managed to develop a direct method of estimating the discrete Normalized Atmospheric Point Spread Function (NAPSF) from available images alone, not using any external sources of information about the atmosphere. ... IRE RAS 1996-20 11 ...

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• Project 4 - RFBR - Stepantsov, Determination of the space anisotropy of order

... Basic Observables: Zero-differenced phase and code ionosphere-free combinations of global GNSS network stations, corrected by P1-C1 satellite code biases (cc2noncc), daily observations with 30 seconds sampling rate Sites coordinates : IGb08 reference frame coordinates and velocities Displacements: solid tides, ocean loading, pole tide loading (IERS 2010) Geometric model : Receivers antennas eccentricities, absolute receiver and ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/tsyba.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm12f.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/pasynok.pdf

THE PHOTOMETRIC RESEARCHS OF THE MERCURY'S SURFACE BY MEANS OF DIGITAL MODELS. ... The surface brightness of Mercury was measured Danjon (1933, 1949, 1953) and Harris (1961) in phase angle 3o-123o. The analysis of the various data of the integral photometric gives the results of determination of the main photometric constants for Mercury. ... THE PHOTOMETRIC RESEARCHS OF THE MERCURY'S SURFACE: S.G. Pugacheva The surface brightness of the Mercurian images was established on the geologic map Mercury. ...

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• Svetlana G. Pugacheva

... SMIS : Space Monitoring Information Support laboratory . Russia's Weather : State Meteorological Center Weather Forecast . Space Weather service : ACE real time solar wind data and simple geomagnetic activity forecast. ... World Fire Web : Space Research Institute (IKI) node . Sputnik : Joint project of SRC Planeta, Rosgidromet and Space Research Institute (IKI) . ... Today's Space Weather : Presented by the Space Environment Center . ... Back to the Space Research Institute Home Page ...

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• ENERGETIC PARTICLE EXPERIMENT DOK-2
• Space Research Institute (IKI) Seminar
• IKI - MSR Research Workshop

URAGAN RELAKSATSIA MOLNIYA-SM VSPLESK IMPULS PLASMA-PROGRESS . ... Progress TCV nominal propulsion system; . ... Determination of parameters (reflecting characteristics, sizes, density etc.) of large-scale plasma formations arising during operation of Progress TCV vernier thrusters and positioning and attitude control thrusters with different directivity of thruster plumes w.r.t. SC motion direction. ... Obtaining of Progress TCV reflecting characteristics in different experiment conditions. ...

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• S.P. Korolev RSC Energia - International Space Station

... CentralProcessor 0.11 documentation . ... Here we detail the input parameters that cover the overall process control, and the switches to turn on & off different parts of the pipeline. Values for parameters that act as flags (ie. those that accept true/false values) should be given in lower case only , to ensure comparisons work properly. These parameters affect how the slurm jobs are set up and where the output data products go. ... SUBMIT_JOBS . ... User Parameters - Pipeline & job control . ...

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• Input Parameters to the Self-Calibration Tasks
• THE SCHED INPUT FILES (Includes parameter lists)
• Cosmological Parameter Survey Using the Gravitational Lensing Method

National Space Agency of Ukraine and . ... The Second International Meeting on WARNING Mission . ... Space Research Institute of Ukrainian National Academy of Sciences - National Space Agency, . ... The Head of Scientific committee of the Project “Warning” is DR V.G.Bar`yahtar, Academitian of Ukrainian National Academy of Sciences. ... Lviv Center Space Research Institute of Ukrainian National Academy of Sciences, . ... National Space Agency of Ukraine, Bozhenka St. 11, 252022 Kyiv-22, Ukraine. ...

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• Researches of Astronomy and Space Physics Department
• Publications of Astronomy and Space Physics Department
• SPECTRUM ANALYZER OF MAGNETIC PHENOMENA SAMW

Monte Carlo Methods for Including Calibration Uncertainties in Model Fitting Analyses Jeremy J. Drakea , Peter Ratzlaffa , Vinay Kashyapa , Richard Edgara , Rima Izemb , Diab Jeriusa , Herman ... University, Cambridge, MA 02138 MIT Kavli Institute for Astrophysics and Space Research, Cambridge, MA 02139 b c SUMMARY · Instrument response uncertainties almost universally ignored in astrophysical X-ray ... Limiting accuracy of Chandra ACIS reached in spectra with 10 4 counts. ...

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• Parameters
• Model Spectra for Spectral-Fitting Program
• SAO RSDC Home Page - RRA

Next: Program use Up: Description of program searchdup Previous: Description of program searchdup . Parameter input is done with a graphic user interface. ... Input file: Name of the input catalog file. It has to be formatted, one record per source/observation, according to the format used in the Arcetri observations and source archives. ... Minimum number of observations per source Source with less than this number of independent observations are not included in the output file . ...

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• Arcetri Star-formation Group Research Topics
• Hubble Finds Oxygen Atmosphere On Jupiter's Moon Europa
• Arcetri Solar Physics Group - Corona and Solar Wind

Main News Phones Research area Brief history Institute Structure Experimental Base Observational data English/Russian . research on the site(Google) . ... 7(4112)390400 . Fax: . 7(4112)390450 . ... Fax: +7(4112) 39-04-50 . Field of investigations: . ... study of global geomagnetic response to sharp variations of parameters of solar wind and interplanetary magnetic field; study of the relation among auroral electrojets, field-aligned currents and a ring current . ...

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Magnetic stars, 2004,225-229 Averaged magnetic phase curves. ... ANALYSIS OF THE CATALOG 227 4 3 N stars 2 1 -4000 -3000 -2000 -1000 0 1000 2000 B0 (G) Figure 3: Number distribution of stars vs. coeffcient B0 for those stars which exhibit a magnetic phase curve with a double wave. of a magnetic star can occur if the angle between the magnetic and rotational axes is small or even zero. ... The catalog lists phase curves for 139 stars, 134 of them are magnetic Ap stars. ...

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• http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2006/riechers_etal_oh104.9+2.4_eso05.pdf
• RESEARCH PROBLEMS of the LRS
• Optimization of spectroscopic observations

Next: C.S. Jeffery, Research Astronomer Up: Research Previous: J.E. Chambers, Research Astronomer Contents . During 1998 Dr Gerry Doyle was involved with three PPARC PDRA research grants, and was also a co-organiser of two international conferences (the COSPAR Symposium `Activity Observed in the Sun and in Similar Stars', and the Armagh Cool Star Workshop `Solar and Stellar Activity: Similarities and Differences'). He was Associate Scientist with the CDS and SUMER instruments on SOHO. ...

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• Irregular Satellite Research
• Armagh Observatory
• C.J. Butler, Research Astronomer

Dynamical chaos in the problem of magnetic jet collimation O. Yu. ... In the paper of Bisnovatyi-Kogan (2007) magnetic collimation resulting from torsional oscillations of a cylinder with elongated magnetic field and periodically distributed initial rotation around the cylinder axis was considered. ... Space and time periods of oscillations depend on the conditions of jet formation: the length-scale, the amplitude of the rotational velocity, and the strength of the magnetic field. ...

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• Zeldovich-100 / International Conference / Moscow, Russia
• Zeldovich-90: COSMOLOGY AND HIGH ENERGY ASTROPHYSICS
• The 6th INTEGRAL Workshop "The Obscured Universe"

... The technology needed to implement a Distributed Astronomical Data Archive (DADA) is available today (e.g., Fullton 1993). Query interface standards are needed, however, before the DADA information will be discoverable. ... These parameters would be used to index each dataset in each catalog. ... The technology is available today to perform cross-catalog queries, to fetch the data at the click of a mouse, quickly to add new observation catalogs, and to distribute the load across multiple machines. ...

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• The VLT Science Archive System
• A Spectroscopy Exposure Time Calculator for IRAF
• Modern CCD Observations of Moving Celestial Objects: Algorithms and Software

P.N. Lebedev Physical Institute Astro Space Center Russian Academy of Sciences S.A. Lavochkin Association, Roscosmos RADIOASTRON The Ground ­ Space Interferometer: radio telescope much larger than the Earth The Spectr-R Project http://www.asc.rssi.ru/ radioastron / High- Resolution HI 21 cm Mosaic of M 33 galaxy GENERAL OUTLINE The RadioAstron ... Such forecast could be used to prepare a long time-scale schedule of scientific observations. ...

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• Parameters of the Moon-perturbed orbit
• ASC home page
• MILLIMETRON

... When using a multidimensional parameter space, it is often impossible to establish frame bounds daubechies:CBMS on the energy in the parameter space. With only one parameter, we cannot always reconstruct the signal. ... To the extent that multi-dimensional parameter spaces are still useful, we will not let this infinite energy hinder our progress...``time-frequency-scale-chirprate . ... In general, g ( t ) is a complex-valued function of a real variable, and has finite energy: 6#6... affine . ...

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• V.A.Baturin - Home Page at Sternberg Astronomy Institute, MSU
• Tutorial on Fortran 90, Digital UNIX
• Миронова Ирина. Mironova Irina Home page

Peremennye Zvezdy", . ... Star Name: . GSC 4487-00399, . ... During observations of GSC 4487-00347, a new eclipsing binary star with an eccentric orbit (Otero et al. 2006), we discovered variability of GSC 4487-00399. ... We suggest that the star is a close-binary EW-type variable with the ephemeris: . ... Light Curve . The spectral window (1a), the power spectrum (1b), and the phase diagram (1c) of the variable star GSC 4487-00399. ... The finding chart for the variable star GSC 4487-00399. ...

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