Next: A Gravimagnetic Rotator Up: No Title Previous: Special Cases: Supernova Explosion . One of the most important achievements in astrophysics during the period 1968-1970 was the realization that in addition to ``ordinary'' stars which derive their energy from nuclear reactions, there are objects in the Universe whose radiation is caused by a strong gravitational and magnetic field. ... Evolution of Magnetic Rotators . ... Evolution of Magnetic Rotators in Non-circular Orbits . ...

... Supervisor: Dr. Luca Del Zanna . ... Parma Workshop on Numerical Relativity and Gravitational Waves, 7-9/09/2011, INFN Parma e Dipartimento di Fisica, Parma . ... 8th Advanced School on Parallel Computing "PRACE Winter School", 6-10/02/2012, CINECA SuperComputing Application and Innovation Department, Bologna . ... Internship "PRACE Winter School Stage", 25/06/2012 - 28/09/2012, CINECA SuperComputing Application and Innovation Department, Bologna . ...

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... In the presence of only uniform magnetic field B , the motion of a charged particle can be described with gyration about the guiding center and motion along the field line. ... In the precence of both magnetic and electric fields, the equation of motion for charged particle (mass m, charge q) is m d v /dt = q ( E + v x B ). ... Because v is independent of the mass and sign of the charge, it is the same for negatively and positively charged particles, and does not create electric current. ...

. Next: Strong Equivalence Principle: Solar Up: Binary Neutron Stars Previous: Constancy of the Chandrasekhar . љ . Each line of sight to a pulsar is analogous to one arm of LIGO, GEO or LISA. Constrain energy density of Gravitational Waves of frequency = 1/data span, ie Hz. Assuming kms Mpc . - Kaspi et al 1994 . Jon Bell . Thu Dec 19 15:15:11 GMT 1996

e-mail: podgorny@inasan.ru . Institute of Astronomy RAS . ... Spectrum of solar flare protons // Journ. ... The active region magnetic flux correlation with flare appearance. ... Podgorny A. I., Podgorny I. M. Solar Flare Numerical Magnetohydrodynamic Simulation and Solar Flare Model. ... Podgorny A. I., Podgorny I. M. MHD simulation of magnetic field configuration above the active region NOAA. ... Podgorny I. М., Podgorny A. I. The active region magnetic field association with solar flares. ...

... V.N. Obridko . ... Oscillations . ... Solar cycle . ... Solar Corona . ... webmaster@izmiran.ru . ... B.A. Ioshpa, V.N. Obridko, B.D. Shelting . ... Solar Physics 29 (1973) 385-392. ... Quasi-biennial oscillations of the global solar magnetic field . ... Quasi-biennial oscillations of the solar global magnetic field . ... Quasi-biennial oscillations of the Solar magnetic fields . Proc. 10th European solar physics meeting",Solar variability: from core to outer frontiers", Prague, Czech. ...

Cherechukin A.A., Koledov V.V., Shavrov V.G., Tulaikova A.A., Vasil'ev A.N. Magnetic and structural phase transitions in Ni2+УMn1-УGa (0<У<1) alloys are investigated experimentally. The martensite domains formation under the action of external magnetic field on the surface of polycrystalline Ni2,19Mn0,81Ga specimen was investigated by optical method. ... It is found that the martensite phase formation temperature is enhanced by the order of 0,3 K in magnetic field of 1 kOe. ...

SPECTRUM ANALYZER OF MAGNETIC PHENOMENA SAMW . Spectrum analyzer allows onboard computation of electromagnetic waves spectra registered (observed) in the ionosphere and magnetosphere in the ELF/VLF frequency band. ... It consists of magnetic antenna, preamplifier, 16 bit sigma delta AD converter, DSP processor and telemetry interface. ... The channels of lower frequencies are averaged and transmitted with lower repetition rate so the telemetry volume is reduced. ... Dynamic range: 90 dB . ...

... Science Users Information > Science Activities > Science in Garching > Research Area: STELLAR STRUCTURE AND EVOLUTION . ... Reset view all 3 per page 5 per page 10 per page Sort by Title A-Z Title Z-A Date asc Date desc Research Topics Planets and Star Formation Stellar Structure and Evolution Stellar Populations Cosmology and the Early Universe Scientific Positions Faculty Fellows Scientists Students . ... Planets and Star Formation Stellar Populations Stellar Structure and Evolution Faculty . ...

... Shkolni bulvar 19/144, Chernogolovka, Moscow distr., ... Institute of Solid State Physics RAS, Chernogolovka. ... Trainee, Institute of Solid State Physics RAS, Chernogolovka. ... Senior Research Scientist, Institute of Solid State Physics RAS, Chernogolovka, Moscow district, Russia. ... Research Scientist, Institute of Solid State Physics RAS, Chernogolovka, Moscow district, Russia. ... Junior Research Scientist, Institute of Solid State Physics RAS, Chernogolovka, Moscow district, Russia. ...

... 2012/11/28 . Bayesian inference of T Tauri star properties using multi-wavelength survey photometry . ... A Volume Limited Radio Survey of Ultracool Dwarfs . ... A high-resolution spectropolarimetric survey of Herbig Ae/Be stars I. Observations and measurements . ... Evolutionary models for double helium white dwarf mergers and the formation of helium-rich hot subdwarfs . ... On the incidence of weak magnetic fields in DA white dwarfs . ... Magnetic fields in central stars of planetary nebulae? ...

... Files in red?history) . ... Field Lines . ... EM Waves . ... Magnetic field lines similarly describe the structure of magnetic fields in three dimensions.They are defined as follows. ... Maxwell Most scientists nowadays view field lines as intangible abstractions, useful only for describing magnetic fields. ... Maxwell also showed (perhaps his greatest achievement) that an "electromagnetic wave" was possible, a rapid interplay of electric and magnetic fields spreading with the velocity of light. ...

In accreting binary neutron star systems matter is channelled by the strong magnetic field to the poles of the neutron star. The accreted matter accumulates at the poles to form accretion mounds. Pressure from the confined matter can significantly distort the local magnetic field structure, affecting the X-ray observations and long term evolution of the magnetic field. ...

National Aeronautics and Space Administration . ... Gregory Errol Chamitoff (Ph.D.) . NASA Astronaut (Former) . ... NASA EXPERIENCE: In 1995, Dr. Chamitoff joined Mission Operations at the Johnson Space Center, where worked as a Guidance and Control Flight Controller. ... SPACE FLIGHT EXPERIENCE: Expedition 17/18 - In 2008, Dr. Chamitoff served as the flight engineer and science officer for a 6-month mission aboard the International Space Station during Expeditions 17 and 18. ... OCTOBER 2013 . ...

... Астронет | ... The second congress of the astronomical society of the former soviet union . ... Modelling the atmospheres of accretion disks . ... The distribution of old neutron stars in the galaxy . ... Compton scattering in a strong magnetic field: Resonances in the cross sections . ... Preface: "Physics of Neutron Stars" . ... Electric fields of neutron stars . ... Magnetic field decay in neutron star cores . ... The non-thermal mode of disc accretion onto the magnetosphere of a neutron star . ...

... The storm began quite unexpectedly. The strongest geomagnetic storm for the last seven months began on Earth almost precisely at the same time as the solar eclipse reached its maximal stage, the culmination of which occurred at GMT 02:35 (06:35 Moscow time). ... Oscillations of such amplitude in the magnetic field have not been observed since October, 11th of last year, which is more than seven months ago. ... We can only add that the magnetic storm lasted approximately 9 hours. ...

... Units are separated by spaces, positive numbers denote powers, all units to the right of the slash are in the denominator (negative powers). Planck constant h . ... 6.0221367e23 particles/mol . ... Free electron gyromagnetic ratio gamma e . ... gamma p / (2 pi) = 42.576375 MHz/T . ... Gas constant R . ... The NIST Reference on Constants, Units, and Uncertainty . CODATA Internationally recommended values of the Fundamental Physical Constants . ... Table of Fundamental Physical Constants (MIT) . ...

... The evolution of magnetic fields in OB-type stars from the study of open clusters of different ages . ... Wade G. A. The MiMeS Project: Magnetism in Massive Stars . ... Polosukhina N., Shavrina T., Drake N., Kudryavtsev D. Smirnova M. New results of the spectral observations of CPstars in the Li I 6708? spectral region with BTA telescope of SAO RAS . ... Magnetic Stars-2010 . ... List of participants . List of reports . ... Laboratory for the Stellar Magnetism Study of SAO of the RAS . ...

... Пширков М.С. Попов С.Б. A new method is suggested to search for axions constituting Dark Matter that utilizes observations of neutron stars (NS) in radio-frequency region. ... For example, if the coupling constant of photon-axion interaction is GeV and the density of DM axions is , then the flux density of excess signal for axions with rest mass of eV will be as large as several tenth of Jy at the frequency 240 MHz in the bandwidth 0.5 MHz. ...