... V.F. Gantmakher, M.V. Golubkov, V.T. Dolgopolov, G.E. Tsydynzhapov and A.A. Shashkin, Pis'ma v ZhETF 68 (4), pp. ... Online version : cond-mat/9807332 . ... V.F.Gantmakher, M.V.Golubkov, V.T.Dolgopolov, G.E.Tsydynzhapov, and A.A.Shashkin . ... V.F.Gantmakher, M.V.Golubkov, V.T.Dolgopolov, G.E.Tsydynzhapov, and A.A.Shashkin, Pis'ma v ZhETF 71 (4), pp.231-237 (2000) . ... V.F.Gantmakher, M.V.Golubkov, V.T.Dolgopolov, A.A.Shashkin and G.E.Tsydynzhapov, Pis'ma v ZhETF 71 (11), pp.693-697 (2000) . ...

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• Electrons in Disordered Media
• LPCBC: Abstract 2_22
• LEK - Equipment

... The quench rate is varied over 4 orders of magnitude. ... The setup Sample geometry Sample holder Thermal cycling Challenges ЇMeasuring cooling rate at T=TC ЇReproducible cycles within several decades of cooling rates ЇNo electrical connections during transition time Quench time: Q = -TC (dT/dt| T=TC) -1 Magnetic fields The effect of an applied orthogonal magnetic field on trapping rate is studied. ... A minimum is expected at zero net field. ... References [1]T. W. B. Kibble, Phys. Rep. ...

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• http://www.cplire.ru/html/lab234/pubs/2006_8.pdf
• http://www.cplire.ru/html/lab234/pubs/2009-13.pdf
• http://www.cplire.ru/html/oxide233/publication09/confTD-P20-4-6.pdf

Pulsars can be used to study the strong nuclear force. The density of matter at the center of neutron stars is one or two orders of magnitude larger than the density of atomic nuclei. ... Very "soft" EOSs predict lower pressures for a given density, i.e., highly compressible matter. ... If more precise measurements can confirm this high value, then many model EOSs for dense matter can be ruled out. ... Another way of studying the behavior of super-dense matter is to find fast pulsars. ...

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• Chapter 11. Specifying OpenGL Environment Variable Settings

The aromatic features in M101 were studied spectroscopically and photometrically using observations from all three instruments on the Spitzer Space Telescope. The global SED of M101 shows strong aromatic feature (commonly called PAH feature) emission. ... This implies that the weakening of the aromatic emission in massive star-forming regions is due primarily to processing of the dust grains in these environments, not to differences in how they form. ...

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• Strange Attractors - Chaos & Fractals
• The Butterfly Effect - Chaos & Fractals
• FOC Linearity

. This diagram illustrates the behavior of margins, borders, and padding at the split points of an inline box. The illustration shows the rendering of the HTML example preceding the image in the main document, the paragraph "Several emphasized words appear here." The inline box containing the words "emphasized text" is split between the words. At the split point, padding, borders (dashed to emphasize them), and margins are not rendered. Return to image.

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... comedi_set_global_oor_behavior -- out-of-range behavior . ... int comedi_set_global_oor_behavior (enum comedi_oor_behavior behavior); . ... This currently affects the behavior of comedi_to_phys() when converting endpoint sample values, that is, sample values equal to 0 or maxdata. If the out-of-range behavior is set to COMEDI_OOR_NAN, endpoint values are converted to NAN. If the out-of-range behavior is set to COMEDI_OOR_NUMBER, the endpoint values are converted similarly to other values. ...

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• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Physics and
• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Home
• Cosmological Gene project

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... A sketch for the active region model on ultracool dwarfs. ... An active region model was built, based on the rotation of the UCD and the ECMI mechanism. ... The active region model is applied to the radio emission from TVLM 513-46546, in which the ECMI mechanism is responsible for the radio bursts from the magnetic tubes and the rotation of the dwarf can modulate the integral of flux with respect to time. ...

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• Abstract

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• U of O High Energy Physics Seminars
• Thermodynamics
• El Nino

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-90: COSMOLOGY AND HIGH ENERGY ASTROPHYSICS

Next: The Present Situation in Up: No Title Previous: Case A: . Why it is possible that the Oppenheimer-Volkoff limit exceeds ? ... The lifetime of HSP (``hot'' spinar) is completely determined by the cooling time which is of the order of s according to different calculations. ... It seems very attractive to identify this cooling time with the mean characteristic gamma-ray burst duration s! . ... Finally, for the high Oppenheimer-Volkoff limit for the cool non-rotating object, when . ...

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• The Stopping Radius
• Ejector-propeller hysteresis
• The Environment of the Rotator

... Apache HTTP Server Version 2.2 . ... Additional functionality allows webmasters to configure the response of Apache to some error or problem. ... If a script crashes and produces a "500 Server Error" response, then this response can be replaced with either some friendlier text or by a redirection to another URL (local or external). ... Custom Error Responses and Redirects . ... In addition to these new variables, Apache will define REDIRECT_URL and REDIRECT_STATUS to help the script trace its origin...

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• Mars Surveyor '98 Orbiter
• Educator's Guide to Sunspots
• Cassini

... Apache HTTP Server Version 2.2 . ... Additional functionality allows webmasters to configure the response of Apache to some error or problem. ... If a script crashes and produces a "500 Server Error" response, then this response can be replaced with either some friendlier text or by a redirection to another URL (local or external). ... Custom Error Responses and Redirects . ... In addition to these new variables, Apache will define REDIRECT_URL and REDIRECT_STATUS to help the script trace its origin...

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• CMOS tutorial-results

spaceweb@oulu.fi - last update: 1 July 1998, 1200 UT (RR) . ... Relates the wave number k to the wave frequency. ... From the equation of motion , m d v /dt = q( v x B ) one can calculate that, in a presence of magnetic field B , a charged particle is accelerated in direction perpendicular to both v (perp) and B . ... The angle a between magnetic field B and velocity vector of a charged particle, v ., i.e., sin a = v(perp) / v(total), where v(perp) refers to the velocity component perpendicular to B . ...

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• List of currently available KP AZ.
• Space Physics Group of Oulu
• Space Weather Dials Interpretation Guide

Main plasma parameters for inhomogeneous plasma. ... Particle motion in the Earth dipole magnetic field. ... Bounce frequency and bounce motion in the Earth inner magnetopshere. ... Low- frequency electrostatic waves in inhomogeneous low- beta plasma. ... Kinetic drift instability. ... Permittivity tensor for electromagnetic low- frequency waves in inhomogeneous low- beta plasma. Drift Alfven waves. ... Spectra of electromagnetic low- frequency waves in inhomogeneous medium- beta plasma. ...

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• Theoretical Astrophysics
• SET OF MAGNETIC AND ELECTRIC FIELD DETECTORS EXO-EM
• ENERGOSPECTROMETER OF IONOSPHERIC PLASMA P3-3

... Future seminars . ... Nonlinear theory of mirror (diamagnetic) instability near its excitation threshol d " . ... It is demonstrated that near threshold of mirror instability the main contribution to the quadratic nonlinearity is connected with perpendicular pressure. We derive the three-dimensional equation which describes the weakly nonlinear behavior of the system. ... As a consequence the corresponding free energy decreases in time providing a blow-up appearance of magnetic holes. ...

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• The Solar Wind
• Magnetic Field Lines
• Magnetic Field Lines -- History

... Observing . ... Star Atlas . ... The shocking behavior of a speedy star . ... Such structures are called bow shocks, and they can often be seen in front of the fastest, most massive stars in the galaxy. ... Slow-moving stars like our Sun have bow shocks that are nearly invisible at all wavelengths of light, but fast stars like Kappa Cassiopeiae create shocks that can be seen by Spitzer's infrared detectors. ... Only registered members of Astronomy.com are allowed to comment on this article. ...

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• Space station provides insight into flame behavior | Astronomy.com
• Cloud behavior expands habitable zone of alien planets | Astronomy.com
• New theory explains supernovae behavior | Astronomy.com

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . ... ISS Russian Segment . ... ISS 45/46 . ... check for the following onboard the ISS RS: a capability to demonstrate the action of physical laws of dynamics of reactive and gyroscopic forces on ellipsoid (Letauschaya Tarelka device) rotating in the unsupported medium in microgravity, with video record of its behavior in the station module; . ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

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• INTERNATIONAL SPACE STATION

... Irreducible and full set of independent orthogonal dimensionless parameters in the `velocity normalised basis' Symbol M Ma Name Mach number Magnetic Mach ( Mach ґ AlfvИn) Strouhal Trieste numbers ( set ) Velocity-emission Formula / Definition Signifiance Temperature Governing MHD equations with dissipation and radiation v v c s S V vt x Magnetic ... DOI: 10.1016/j.asr.2005.03.084 ...

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• APEX/Intro
• Non-traditional methods of geophysical investigations and active plasma
• APEX/Equipment

... Amorphous carbonaceous materials can show a great diversity of optical properties due to the variability in their microstructure. ... The differently pyrolized celluloses are representative for a suit of carbonaceous material ranging from strongly disordered (insulating) to graphitized (conducting) material. Figure: Complex refractive index of hydrogenated amorphous carbon prepared by pyrolysis (annealing) of cellulose at different temperatures. ...

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H 2 O maser sources spectral data at 22 GHz. I began this project 27.08.1998 for displaying spectral data at 22 GHz of water maser. While data will concerning in base Puschino many year (1979-1998 yy) regular observations of sample of these sources. Sources . R.a. (1950.0) . ... The figures with many years spectral data (day-month-year) . The behavior of flux . The behavior of spectral components . ... All spectra 1981-94 . ... The some spectral component: many year behavior . ...

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