Describes how spatial region boundaries are handled. The golden rule for spatial region filtering was first enunciated by Leon VanSpeybroeck in 1986: . ... With this in mind, the rules for determining whether a boundary image pixel or table row are assigned to a region are defined below. For image filtering, pixels whose center is inside the boundary are included. ... That is, an row is inside the boundary without regard to its integerized pixel value. ...

... Observations of precipitating (Jp) and trapped (Jt) energetic (> 30 keV) particle fluxes at the ionospheric altitudes within the auroral oval region has revealed the existence of a sharp boundary separating the poleward zone of isotropic precipitation (Jp = Jt) from the equatorward zone of weak loss cone filling (Jp << Jt) at all local times (Sergeev and Malkov, 1988). ... boundaries for higher energy particles are located at lower latitudes than boundaries for lower energy particles . ...

Next: Blinkers and Bi-directional Jets Up: J.G. Doyle, Research Astronomer Previous: J.G. Doyle, Research Astronomer . Gerry Doyle reports that collaborative research with Maria Madjarska has revealed for the first time the presence of bi-directional jets and magnetic reconnection occurring at coronal hole boundaries. ... Next: Blinkers and Bi-directional Jets Up: J.G. Doyle, Research Astronomer Previous: J.G. Doyle, Research Astronomer M.E. Bailey . ...

Next: TAPE LENGTHS and PASS Up: Tape Management Previous: GENERAL CONCERNS Contents . There are a number of concerns related to tape handling at scan boundaries. ... Between scans, tapes can be kept running or can be stopped. ... But if it has many short scans, such as when phase referencing, it can be highly advantageous to keep the tape moving between scans. ... If there are long gaps (many minutes) between scans, tape use efficiency is enhanced if the tapes are stopped. ...

. Proceedings of Turbulent Shear Flows XI, Sept. 1997. Jacques Lewalle, jlewalle@syr.edu

Astronomy Picture of the Day . Jupiter: At The Belt-Zone Boundary . ... 9.03.1997 . ... Credit Copyright: The Galileo Project , JPL , NASA Explanation: Jupiter's thick atmosphere is striped by wind-driven cloud bands that remain fixed in latitude - dark colored bands are known as belts while light colored bands are zones. At Jupiter's belt-zone boundaries the shearing wind velocities can reach nearly 300 miles per hour . ... March 1997 . ... Publications with keywords: Jupiter . ...

Galileo Crosses Boundary Into Jupiter's Environment . NASA's Galileo spacecraft radioed confirmation late this week that it has entered Jupiter's environment, crossing over the boundary from interplanetary space into the giant magnetic cocoon around Jupiter called the magnetosphere. ... On Thursday, December 7, Galileo's previously deployed atmospheric probe will plunge into Jupiter's cloud tops at 5:56 p.m. EST and descend into the giant planet on a parachute. ... Space History Galileo . ...

Name Last modified Size Description . Parent Directory - Erkaev.ppt 30-Mar-2009 19:54 1.1M Grib.ppt 30-Mar-2009 19:54 1.9M Koinash.ppt 30-Mar-2009 19:54 1.0M Rossolenko.ppt 30-Mar-2009 19:54 817K Verigin.ppt 30-Mar-2009 19:54 920K .

... Tonight's Sky . ... SET т?? ... Observing . ... Astronomy for Kids . ... Observing springtime deep-sky objects with a large telescope . ... How were the constellation boundaries set? They appear pretty arbitrary. ... If you think the constellation boundaries look arbitrary now, consider the situation a century ago. ... Get instant access to subscriber content on Astronomy.com! ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ...

... Designation used on the ASCII files . Designation used on the plots . ... Low Latitude Boundary Layer . ... High Latitude Boundary Layer . ... Tail Northern Lobe . ... LOBS . Tail Southern Lobe . ... Polar Cap . ... CAP . Cusp . ... CUSP . ... AUR . ... See as well the used simulative magnetosphere's regions and boundaries models . ...

Chair of solid state physics . ... Defects in crystals . ... Lectures program for the undergraduate students of the Faculty of general and applied physics of Moscow Institute of Physics and Technology (State University) . The defect-free and unlimited solid is though a useful ideal construction, but it is quite far from reality. ... At the beginning, the 0-dimensional defects like vacancies, interstitials, dislocation kinks and kinks of surface steps are discussed. ... Grain boundary dislocations. ...

... autoOutline (int startX, int startY) . ... 0 and the boundary points can be accessed in the public xpoints and ypoints fields. public void autoOutline (int startX, int startY, double lower, double upper) . 0 and the boundary points can be accessed in the public xpoints and ypoints fields. public void autoOutline (int startX, int startY, int lower, int upper) . This is a variation of legacy autoOutline that uses int threshold arguments. public void autoOutline (int startX, int startY) . ...

... The light from hundreds of billions of stars in a galaxy has combined to fill this new space picture with a soft glow. It s hard to see the shape of this galaxy because its light gently fades away as you move away from the centre, with no solid boundary to mark the edge. ... Astronomers call galaxies with this shape ellipticals. ... Our Galaxy, the Milky Way, is a spiral galaxy.) Ellipticals are the biggest galaxies in the Universe and their stars orbit around the centre in all directions. ...

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... научных трудов Кочетковой А.Ю. Postnov K. A., Shakura N. I., Kochetkova A. Yu., ... Shakura N. I., Postnov K. A., Kochetkova A. Theory of wind accretion. ... Postnov K., Shakura N., Staubert R., Kochetkova A., Klochkov D., Wilms J. Variable neutron star free precession in Hercules X-1 from evolution of RXTE X-ray pulse profiles with phase of the 35-d cycle. ... Shakura N., Postnov K., Kochetkova A., Hjalmarsdotter L. Theory of quasi-spherical accretion in X-ray pulsars. ...

... SMIS ] . PROJECT "FOREST FIRES 96" . ... Moscow . ... Vologda (east part) . ... Komi (north part) . ... Komi (south part) . ... Ural (north part) . ... Ural (south part) . ... Tyumen (north part) . ... Tyumen (south part) . ... Irkutsk . ... Krasnoyarsk (north part) . ... Krasnoyarsk (south part) . ... Irkutsk region (north part) . ... Irkutsk region (west part) . ... Irkutsk region (east part) . ... Chita (north part) . ... Khabarovsk (north part) . ... Sakhalin (north part) . ...

In this method the fields outside and inside a particle are represented by expansions in term of proper basis functions (practically always the vector spherical harmonics). Since the particle surface does not coincide with the coordinate surface, it is impossible to satisfy the boundary conditions exactly, and the expansions are limited by a finite number of terms, and the boundary conditions are considered in a finite set of points (matching points). ...

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Do we need various assumptions to get a good FCN? A new multiple layer spectral method Cheng-li HuangMian Zhang Shanghai Astron. ... No FCN ! ... FCN,FCN,FCN.. Multiple layer spectral method (MLSM) + Linear Operator Method (LOM) Finite Element Method (FEM) · · Traditional approach solves one order ellipsoid only. ... Main Idea of FEM Boundary Surface could be described as: Let's consider how to solve the dynamic equation: Traditional Approach: Equivalent Spherical Domain . ...

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