... Email: chaos@mail.cplire.ru . ... We investigate phenomena on the edge of spatially homogeneous chaotic mode and spatiotemporal chaos in a lattice of chaotic 1-D maps with local connections. We show that spatially homogeneous chaotic mode cannot exist in a lattice with local connections if the Lyapunov exponent of the isolated chaotic map is greater than some critical positive value. We propose a few schemes that make spatial synchronization possible in large lattices. ...

... Posts tagged ?regularity conditions? ... If getting the first derivative (score function) and the second derivative (empirical Fisher information) of a (pseudo) likelihood function is feasible and checking regularity conditions is viable, a test for global maximum (Li and Jiang, JASA, 1999, Vol. 94, pp. 847-854) seems to be a useful reference for verifying the best fit solution. ... 2 Comments . ... Entries RSS . ... vlk on [MADS] Parallel Coordinates . ... Entries (RSS) and Comments (RSS) . ...

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... ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . Mopra radio telescope . ... Australia Telescope Online Archive (ATOA) . ... Parkes | ... Australia Telescope 20GHz Survey . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... Previous Section: APPENDIX A. The composite . ...

The Earth's magnetosphere global structure is conditioned by the interaction of the Solar wind and Earth's magnetic field. ... Many various magnetospheric models are available in the NSSDC . ... Fairfield D. H., Average and unusual location of the Earth's magnetopause and bow shock, J. Geophys. ... Stasiewicz K., Polar Cusp Topology and Position as a Function of Interplanetary Magnetic Field and Magnetic Activity: Comparison of a Model with Viking and other Observations, J. Geophys. ...

function DD= deter(om); global ro go % for boundary condition global omegao2 lorder % global Xfin_i Yfin_i Xfin_o Yfin_o global sol_out sol_in kk_out global r_in r_cut r_out omegao2 =om; r_tp = r_in ^(lorder-1); Y0 = [ omegao2 * r_in * r_tp ; lorder* r_tp ]; opt_ode = odeset('RelTol',3e-5); sol_in = ode45 (@ Diffur , [ r_in r_cut ], Y0, opt_ode ); %[Xfin_i, Yfin_i] = ...

. Russian (WIN) . 10-27/2/1999 . 6-28/1/1999 . For more information send a mail to: info@sputnik.infospace.ru . ? 1998-2002 SMIS IKI RAN and SRC "PLANETA" Moscow, Russia.

home . projects . my portfolio . blog . contact . My Ph.D. work was focused mainly on the development of boundary conditions for Smoothed Particle Hydrodynamics simulations of binary stars. ... I developed and tested an innovative way of modeling only the outer parts of stars, therefore allowing for an increased particle and mass resolution in the mass transfer itself. This work was published in Lajoie Sills 2010a (The Astrophysical Journal 726, 66). ...

... MAO main . ... July Issue: Global Sensor Networks Will Change Human Consciousness . ... Тема: July Issue: Global Sensor Networks Will Change Human Consciousness . ... July 2014 Issue Highlights . ... Scientific American Volume 311, Issue 1 . ... Extra Sensory Perception How a world filled with sensors will change the way we see, hear, think and live . ... Board Categories MAO main - Info - MAO - news - Flame Technical - Technical Support(Forum)(Техподдержка(Форум)) . ... MAO NASU . ...

For solar wind dials without any explanatory text, see this page . ... There are three logs, one for each condition index ( K P , Solar Wind ,and NOAA/SEC .) ... More about the solar wind's recent behavior can be found on my Current Solar Wind Conditions page. ... Other items of interest include NOAA/SEC Current Conditions , my composite current Auroral Images page, Windows on the Universe: Space Weather , and Public Outreach Index, Department of Space Physics and Astronomy, Rice University . ...

... ARC 3.5m | Weather Closure Conditions . The enclosure will be closed by the Observing Specialist under the following conditions. ... This policy will be consulted whenever there are questions or disagreements concerning closure of the APO 3.5-meter telescope due to hazardous conditions or situations, at times when telescope operations are being overseen by an APO Observing Specialist. ... the on-duty Observing Specialist has full responsibility, and sole authority, to make this decision. ...

. Latest HI Rez Visible Satellite Image . IR Enhanced Image of the PNW . (not always available - sorry) . 500 MB surface and the water vapor distribution: . Surface Pressures: . Extreme precipitation in 1995 and 1996 . Temperatures: Jan-Feb , Mar-Apr , May-Jun , July-August , Sept-Oct, Nov-Dec . Precipitation: Jan-Feb , Mar-Apr , May-Jun, July-Aug , Sept-Oct, Nov-Dec . Annual Precipitation Trends . The Electronic Universe Project e-mail: nuts@moo.uoregon.edu

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) Ї Ї 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 . ...

... Assured of a reliable method of solving the normal equations, we now consider the equations of condition. The observed magnitude m of a star at M air masses with true instrumental magnitude is modelled as ([ 10 ], [ 28 ]) . ... The effective extinction coefficient depends on the effective spectral gradient [ 29 ] of the star, for which we use some color index, affected by half the atmospheric reddening ([ 26 ], [ 10 ]): . ... Thus, for the B band of UBV, we use the (U-V) color. ...

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). ...

. Next: Space and velocity distributions Up: Old neutron star distribution Previous: State of the problem . Space and velocity distributions . Space position . Initial velocity . Galactic potential . Mike E. Prokhorov . Fri Jul 19 19:16:07 MSD 1996

... Observatory . ... Science . ... Science Users Information > Science Publications > Reports > Environmental Conditions on ESO Observatories . ... La Silla Paranal Observatory . ... ESO-MIDAS . ... Data Handling and Products . ... Science Data Products Forum . ... ESO Data . ... ESO Data Access Policy . ... ESO Science Newsletter . ... April, May, June 1999 . ... In March and April 1996 anomalies in Paranal weather conditions were experienced - please read the special report. ... April, May, June 1996...

Consequences of Impacts of Cosmic Objects in Circumstances of Changing Climate . ... The consequences of the impacts of asteroids about 1 km in size on the Earth are considered from the viewpoint of their negative effects under conditions when the climate changes. These effects are ejection of greenhouse gases, fires, changes in surface albedo, and global dispersion of asteroid material. ...

... Gallery . ... The PDS and some air-conditioning relics, reaтАж . Sidebar Left . Sidebar Top . No Sidebar . Sidebar Bottom . Sidebar Right . ... Title: The PDS and some air-conditioning relics, ready for junking. Description: NOTE: All images and movies are copyright and must not be reproduced or mirrored in any form without written permission. ... NOTE: All images and movies are copyright and must not be reproduced or mirrored in any form without written permission. ...

... Grant of RFBR #97-05-64085 . ... The project goal is the investigation of the global storm-time variations of electron density and temperature and dynamics of the topside ionosphere structure (day-side cusp, auroral oval, main ionospheric trough, ring ionospheric trough, subauroral Te peak and equatorial anomaly). ... The background Ne distribution at the height of ~430 km for the quiet night-time equinoctial conditions from the Cosmos-900 data is constructed and investigated - Fig.5. ...