The space between the planets is far from empty. It contains: electromagnetic radiation (photons); hot plasma (electrons, protons and other ions) a.k.a. the solar wind ; cosmic rays; microscopic dust particles; and magnetic fields (primarily the Sun's). While the Sun 's radiation is obvious, the other components of the interplanetary medium were not discovered until very recently. ... Except near some of the planets, interplanetary space is filled with the Sun's magnetic field. ... Sun .. ...

Magnetic Stars, 2011, pp. ... We discuss our most recent determination of the rotational period from longitudinal magnetic field measurements and H variability -- the latter obtained from over a decade's worth of professional and amateur spectroscopic observations. ... We concluded that the dipolar field of HD 57682 is characterized by a polar strength of 1.7 kG, and a magnetic axis aligned within 10 to 50 of the rotation axis, depending on the inclination of the rotation axis to our line of sight. ...

... The course is intended to provide an introduction to the field of solar-terrestrial physics to new PPARC postgraduate students (and others) starting work in the fields of solar physics, the solar corona and solar wind, magnetospheric physics and the physics of the upper atmosphere of the Earth. ... The intention is to provide students with an overview of the whole coupled Sun-Earth system. ...

Most current theories for magnetospheric emission can be grouped into polar cap, outer gap, and nebular models. These models, at least in some cases, need not be mutually exclusive; the Crab pulsar (among others), for example, shows clear evidence for pulsed emission from the magnetosphere and unpulsed emission from the surrounding nebula. ... This suggestion is strengthened by observation of a distinct soft emission component, consistent with the cooling scenario, from several of these pulsars. ...

... In electron-positron colliders, effect of the lattice modification by opposing bunch focusing on the equilibrium radiation emittance is important at high values of the space charge parameter, so one should correctly evaluate this dynamic radiation emittance of the weak beam, which may differ a lot from the nominal emittance, already in the linear beam-beam force model. ... The linearized beam-beam force is equivalent to focusing insertion in linear lattice of the collider. ...

... Информация Руководство и преподаватели Башкиров Евгений Константинович . ... Bashkirov E.K. , Mastyugin M.S. The influence of atomic coherence and dipole-dipole interaction on entanglement of two qubits with nondegenerate two-photon transitions // Pramana - Journal of Physics. ... Bashkirov E.K. , Litvinova D.V. Entanglement between two atoms in the presence of dipole-dipole interaction and atomic coherence // Progress in Biomedical Optics and Imaging - Proceedings of SPIE, 2014, , , 2014 г., P. 1-8...

... Recent applications of multi-spectral imaging in auroral research are combining these dimensions, providing a new perspective on the poorly understood physics of magnetosphere-ionosphere coupling. ... He is an Associate Editor for the Journal of Geophysical Research. ... Please join us for a pre-meeting dinner discussion at Changsho, 1712 Mass Ave, Cambridge, MA at 6:00pm before the meeting. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

. Subdwarfs . Metal deficient red giants in galactic field . Red horizontal branch stars . Blue horizontal branch stars . Extended horizontal branch stars . Stars inside globular clusters . W Vir type stars . IRAS-sources identified with peculiar supergiants . RCrB type stars . Sakurai's object . peculiar supergiant FG Sge .

... Pritchard Alejandro Caceres Anthony Challinor Ian Hinder · Papers on www.mrao.cam.ac.uk/~Clifford ­ gr-qc/0106039 ­ gr-qc/0209090 Black Holes 2002 2 Outline · 4 phenomena to give a classical and quantum description for Classical Scattering Absorption Bound states Emission x Black Holes 2002 3 Quantum Classical Scattering · Main method of comparison is the differential cross section pf GM p b i For r-1 potential get Rutherford formula Black ... Black Holes 2002 55 ...

... Authors: Crystal L. Martin Both galaxies and the intergalactic medium evolve dramatically between z 2 and the present. These changes are coupled via galactic winds, cloud accretion, and ionizing radiation. Measurements of these interactions are critical for building a physical understanding of galaxy assembly. ... Rather modest gains in UV sensitivity are shown to produce enormous gains in our ability to follow the very low-density gas dispersed by galactic winds and galaxy interactions. ...

Converts from 3D space to a simpler 2D space – orders by magnetic field line (assumes dipole geometry). McIlwain's shell parameter (L) is a measure of “equatorial radius.” ? labels a field line, even in a non-dipole field. Magnetic Field Intensity (B) – measure of “latitude.” L – Undefined for open field lines. B (static field model) doesn’t sufficiently order the XMM data due to dynamic environment . ... Previous slide . Next slide . Back to first slide . ...

... Product Information . Charge Coupled Devices (CCDs) . ... Hamamatsu CCDs are scientific grade with low dark current MPP operation, eight-electron rms readout noise, and wide dynamic range. ... In general, the photosensitive area of a FFTCCD is completely covered with polysilicon gates for charge transportation. A front-illuminated (FI-CCD) device has no response in the UV spectrum, because the polysilicon gates absorb the input light. ... Ask for the S7010/S7011 series. ... About Hamamatsu | ...

... Fall 2001 . ... With heavy water as its target medium the Sudbury Neutrino Observatory (SNO) is designed to study solar neutrinos by measuring both the total flux of 8B neutrinos through the neutral-current interaction as well as the electron-type neutrino flux via charged-current dissociation of deuterium. By comparing the electron neutrino flux to the total solar neutrino flux, SNO can make a unique study of the solar neutrino deficit and a model independent test for neutrino oscillations. ...

... Shematovich, V.I . ... Shematovich, V. I. ; Bisikalo, D. V.; Marov , M. Ya . ... Shematovich, V.I., Bisikalo, D.V., and Gerard J.-C. Superthermal particles in the planetary atmosphere. ... Shematovich, V.I., Bisikalo, D.V., and Gerard, J.-C. The thermospheric odd nitrogen photochemistry : role of non-thermal N(4S) atoms (abstract) . ... Geophys ., ... Gerard, J.C., Shematovich, V.I., and Bisikalo, D.V. Effect of hot N( 4S) atoms on the NO solar cycle variation in the lower thermosphere (abstract) . ...

... EXPERIMENTS AND RESEARCHES . ... EXPERIMENT "KULONOVSKIY KRISTALL" . ... Study of dynamics of charged macroparticle systems in a magnetic field under microgravity conditions. ... Apparatus KUK. ... Shooting of dust plasma structures is conducted in a magnetic trap. ... Experiment results: . Testing the methods to control dynamics of solid, disperse, liquid media via magnetic field under microgravity conditions. Physical modeling of dynamics of space dust particles exposed to sunlight. ...

... In the western literature this method is now called ``coupled dipole method" (CDM). ... Thus, a system of equations relative to the fields scattered by the elementary domains can be obtained, and summation of these fields gives the total scattering field. ... A subtle difference between both methods is in the fact that in the first method one works with the fields which excite a dipole (without the field of the dipole), whereas in the second method one uses the real fields in a given domain. ...

... 8, ``Celestial Mechanics'', 2002 Dynamic evolution of resonance orbits of exoplanets in system 47 Uma B. R. Mushailov, A. A. Kaloshin Sternberg Astronomical Institute, Moscow, Russia The orbits of the major and minor planets of the Solar system indicate that their dynamic evolution is essentially influenced by the effects of orbital reso­ nance interactions. ... One may expect that the orbital resonances can exist not only in the Solar system, but also in other star systems. ...

Spacecraft STP Data 1. ... This CD-ROM contains solar flare reports, sunspot numbers and regions histories, total solar irradiance, and solar bursts. ... MAGSAT - 2 discs. ... A Compilation of 1963-1999 Solar Wind Field and Plasma Data, Near Earth and Deep Space - 3 discs. This CD-ROM contains the interplanetary magnetic field (IMF) and solar wind plasma (SWP) data from several spacecraft which have explored the near-Earth and deep space regions over the last three decades. ...

. Int. J. Multiphase Flow 21, 467-483, 1995. In preparation, 1995. Int. J. Multiphase Flow 20, 415-437, 1994. Phys. Fluids 6, 3109-3115, 1994. Studies in Turbulence (Gatski, Sarkar, Speziale Eds.) 461-483, Springer-Verlag 1992. AIAA Journ. 28, 106-112, 1990. Jacques Lewalle, jlewalle@syr.edu

... ORAL SESSION . ... Registration /Coffee . ... Sergey Bogachev : Space solar investigations in the Lebedev Institute: from Sputnik-2 to future missions . ... Splinter session. S1 : SOLARIS mission proposal (chair - S.Kuzin) . ... Morning Coffee . ... The Sun from radio to gamma rays: new results from space and ground-based observatories (part 1) . ... Szymon Gburek : SphinX and XRT observations of active regions . ... Artem Ulyanov : Nanoflares in the quiet solar corona: a view from SDO/AIA . ...