... Space Res., 12, 265, 1992 planetary magnetic dipole: Mizutani, H., et al., ... Astrobiology, 7, 167, 2007 CME induced H+ ion pick-up loss at 0.05 AU for ` Hot Jupiters ' HD209458 b Mass loss ~1011 g/s even for weak CMEs Mmax strong magn. protection in reality Exoplanet magnetospheres - importance of magnetodisk Relatively large amount of observed Hot Jupiters (27%): survival of close-in giants indicates their efficient protection against of extreme plasma and radiation conditions ...

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Hide Zen home . ... Index . ... Do we really need them for database indexing ? ... We need simple numbering scheme, so that for any given point we could easily calculate the number of "pixel", this is what HealPix provides and lacks HTM. ... During Rtree queries the number of index blocks read is several times greater than during Q3C queries. ... But in Q3C scheme, as we showed before, the circle is segmented, so we extract from the database only a few percents more data than occur in the circle. ...

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• Sternberg Astronomical Institute
• APOD: 2013 May 19 - Earths Richat Structure
• APOD: 2000 October 8 - Earth's Richat Structure

... Time-dependent diffusion of Fe compared to the equi- librium stratification for a model with T eff = 10 000 K, log g = 4.0 and a magnetic field of 10 kG strength, inclined by 60 with re- spect to the surface normal. ... The dash-dotted line gives the equilibrium stratification - the radiative acceleration of Fe is equal to 4.0 throughout the atmosphere. ... Numerical modelling of surface abundance distributions in ApBp star atmospheres constitutes a challenging astrophysical problem. ...

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• J.G. Doyle, Research Astronomer
• M.D. Smith, Research Astronomer
• Online Talks

... Files with sunspot magnetic fields data ============================================== Column Format Description ______________________________________________ 1-2 I2 Day of month 3-4 I2 Month (numerical) 5-8 I4 Year 9 A1 Blank 10-13 I4 UT in hhmm 14 A1 Blank 15-19 A5 Sc - atmospheric flutter in arc sec 20 A1 Blank 21-25 A5 S - quality of the Sun image 26-27 A2 Blank 28-31 A4 Number of sunspots (numbering from unit every day ) 32 A1 ...

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• Datafile structure
• Enslish version of database
• structure

... The NATO "Science for Peace" Program , Project number SfP 973559 . ... Receiver devices based on superconducting Josephson junction dynamics provide easy and extremely sensitive way for measurements of contents of these molecules. ... Fast development of SQUIDs resulted in fabrication of number of devices for supersensitive physical experiments and production of sophisticated multichannel measurement systems used in medicine for magnetocardiography and neural investigations. ...

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• Project 5 - State Program "Condenced Matter Physics"
• Signal Processing and Telecommunications
• Plasma Chemical Technologies for Processing Materials of Micro- and

... part 2 | ... Part 1 . The new concept of formation and development of the Solar system. ... Thus, the initial pulse of the rotation of a protosolar cloud of the solar system was determined as a result of the diversion of a part of the moment of the rotational pulse of the Galaxy. ... Besides this new approach to the pre-solar system as a system of the destroyed vortex structure, we can understand now a number of other peculiarities of the Solar system's structure. ...

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• The basic stages in the Earth's pre-geological development
• The new circuit of global tectonics of the Earth, planets and satellites.

Next: A Universal Diagram for Up: ``Ecology'' of Magnetic Rotators Previous: The Corotation Radius . The interaction of a magnetic rotator with the surrounding plasma to a large extent depends on the relation between the four characteristic radii: the stopping radius, , the gravitational capture radius,   , the light cylinder radius,   , and the corotation radius,   . ... Hence, the classification of the interaction regimes may well mean the classification of magnetic rotators. ...

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• Seminars
• The Stopping Radius in the Supercritical Case
• The Effect of Relativistic Wind on Accretion Flow Parameters

... A program packet is developed for the detailed research into the 3D structure of the magnetic fields of solar active regions as well as the overall solar magnetic field. ... Solar activity is the result of motion and interaction of the coronal magnetic fields, so their study is of primary interest of solar physicists. We have developed a program packet for the detailed research into the 3D structure of the magnetic fields of solar active regions as well as the overall solar magnetic field. ...

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• A Wavelet Parallel Code for Structure Detection
• Spatial Structure of NGC 6822: An Example for Statistical Modeling of
• Data Structure and Software of the UCAC-S Project

The efficiency of interaction of radiation with a particle and hence its optical properties depend on the particle chemical composition, size, shape, structure, etc. ... Particle size expressed in units of the wavelength of incident radiation, together with chemical composition, most strongly affects the optical properties of a scatterer. ... There are many methods to solve the light-scattering problem for a homogeneous spheroid (our survey of the light-scattering methods see here ). ...

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• Vladimir P. Reshetnikov's Home Page
• Integral equation method
• Model realization and some results

Are Energy Conditions Violated by Expanding Wormholes? ... We have obtained time-dependent so- lutions of the Einstein and Brans-Dicke eld equations which rep- resent evolving wormholes in a radiation-dominated cosmological background. These solutions are classi ed into various groups and studied separately. ... The problem is also studied in the frame- work of the Brans-Dicke theory and conditions for the absence of exotic matter are derived. ...

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• Structure of Active Galactic Nuclei in a model with the radial magnetic field
• 1803+78: A Helical Core Jet
• Graca Rocha - Research

... 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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... теория твердого тела . теория полупроводников . ... Atomic and molecular collision processes and interactions . ... Electronic transport in condensed matter . ... Electronic structure and electrical properties of surfaces, interfaces, thin films, and low-dimensional structures . ... Magnetic resonances and relaxations in condensed matter, Mossbauer effect . ... Optical properties, condensed-matter spectroscopy and other interactions of radiation and particles with condensed matter . ...

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• Korpus expertov: rubrikator po fizike

PARTICLE ACCELERATION , MAGNETIC FIELD GENERATION AND EMISSION FROM RELATIVISTIC JETS AND SUPERNOVA REMNANTS K.-I. Nishikawa1 , D. H. Hartmann2 , P. Hardee3 , C. Hededal4 , Y. Mizunno5 , and G. J. Fishman 1 6 ... and Technology Center, 320 Sparkman Drive, SD 50, Huntsville, AL 35805 ABSTRACT We performed numerical simulations of particle acceleration , magnetic field generation, and emission from shocks in order to understand the observed emission from ...

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• Истомин Яков Николаевич (ФИАН)
• Zeldovich-90: COSMOLOGY AND HIGH ENERGY ASTROPHYSICS

Japan/USA/England Solar Probe . ... The objective of Yohkoh (Japanese for sunbeam) is to study the high-energy radiations from solar flares (hard and soft X-rays and energetic neutrons) as well as quiet structures and pre-flare conditions. The mission is a successor to Hinotori, a previous Japanese spacecraft flown at the previous solar activity maximum in 1981. Yohkoh was launched on August 30, 1991. ... The Yohkoh mission is a cooperative mission of Japan, the US, and England. ...

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• Arcetri Solar Physics Group: Solar Polarimetry
• AO on AR 8970
• Space spaghetti in magnetic sauce

... V.V.Shevchenko, Sternberg State Astronomical Institute, Moscow University, Universitetsky 13, Moscow 119899, Russia, shev@sai.msu.ru . ... 1.Sternberg State Astronomical Institute, 119899, Moscow, Russia. shev@sai.msu.ru . ... V.V.Shevchenko, Sternberg State Astronomical Institute, Moscow University, Moscow 119992, Russia, shev@sai.msu.ru . ... 119992 Moscow, Russia; . ... 2Sternberg Astronomical Institute, Moscow University, Moscow, 119992, Russia, . ... Moscow, 119992, Russia shev@sai.msu.ru . ...

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... 8, ``Celestial Mechanics'', 2002 Parameterization of the Solar Radiation Pressure model for GPS satellites I. S. Gayazov Institute of Applied Astronomy, St. Petersburg, Russia The treatment of solar radiation pressure (SRP) effect until now is the main problem in precise modeling of GPS satellite orbits. ... In practice, however, all seven parameters of the empirical model cannot be confidently determined from phase observations. ... Bar­Sever Y. E. A new model for GPS yaw attitude. ...

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• http://www.ipa.nw.ru/conference/2002/sovet/PS/FOMINOV.PS
• Keywords_157

RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . General information Main characteristics of the Radio telescope Observing programs General view of the antenna array Main research areas Principle of generation of radio images Radio telescope 's beam Receiving systems Main characteristics of the base receiving-recording complex Calibrations Data archive and databases Publication SSRT - Siberian Solar Radio Telescope . ...

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TOOLS OF TEST GENERATION FOR SATELLITES CONTROL PROGRAMS Andrey Tyugashev, Ekaterina Myasnikova, Elena Sopchenko S.P. Korolyov Samara State Aerospace University (National Reseach University) The paper presents a research in the field of test automation for testing spacecraft control programs. ... Programmers or designers of spacecraft systems write tests manually. ... Tests are carried out by issuing the control actions on the spacecraft and condition monitoring systems parameters of the spacecraft. ...

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• Semkin Nikolay Danilovich
• СГАУ - Topological types of crystal structures
• Murzin Sergey Petrovich

... Centrifuge . ... The major factor of the orbital flight, affecting a cosmonaut, is a weightlessness state, which causes essential changes in cardiovascular and vestibular systems operation. ... In addition, you can experience a long-term G-load in a desirable value and direction, including simulation of the typical test profiles for fighter - pilots and cosmonauts. ... Info: Industry news On-line Data Company ATLAS news Events We in press Contact . Copyright 2000-2016 ATLAS Aerospace . ...

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• Scuba diving in International Space Station model in space suit ORLAN M.

... OFFSET (chan) . GAIN (eV/chan) . RAND_MIN= 0.00000000000000E+00 / lower limit for PHA randomization RAND_MAX= 1.00000000000000E+00 / upper limit for PHA randomization QSPLITR2= 1.00000000000000E+00 / charge split ratio for 2-pixel events QSPLITR3= 1.00000000000000E+00 / charge split ratio for 3-pixel events QSPLITR4= 1.00000000000000E+00 / charge split ratio for 4-pixel events ALGOID = 1 / CAL algorithm identifier REFTIME = '2001-11-05T20:00:00' / reference for parameterization of offset . ...

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• EllipseT structure definition
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