... 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. ...

Subject, Problems and Objects of Theoretical Astrophysics. ... Stellar Photospheres, Their Features. ... Physics of Continuous Radiation Absorption in Stellar Photospheres. ... Continuous Radiation Absorption in Stellar Photospheres of Various Spectral Classes. Solar Type Photospheres. ... Characterisics of Absorption Lines. ... Interstellar Absorption Lines, Their Features. ... Physical and Dynamic Features of Interstellar Medium, Which Follows from Observations of Interstellar Absorption Lines. ...

The Australia Telescope Compact Array (ATCA) . Home page Team Galaxy Sample Observations Papers Projects Related Surveys Pipeline Meetings . Local Volume galaxies ( B. Koribalski) . The Local Volume HI Survey'' (LVHIS) is a project comprising deep HI line and 20-cm radio continuum observations for all nearby, gas-rich galaxies, supplemented by multi-wavelength data. ... Our aim is to study the formation and evolution of galaxies in the Local Universe. ...

... Jan-February: Very mild with only 5 days in the period . ... March 11: 71 degrees - ties record high . ... May 8-17: Icky weather: Highs never about 55 . ... Eugene Record 24 hr rainfall on May 29: 1.05 inches . Salem new record rainfall for month: 5.55 inches . Portland new record rainfall for month: 5.55 inches . ... 14 days with highs less than 60 for Eugene . ... Record Highs: July 26 = 102; July 27 = 105 . ... New Drought Record: 84 days: June 26 - Sept 15 . ...

... 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. ...

Physica B 284}288 (2000) 649 } 650 Superconductor}insulator transition in amorphous In}O lms V.F. Gantmakher*, M.V. Golubkov, V.T. Dolgopolov, G.E. Tsydynzhapov, A.A. Shashkin Institute of Solid State Physics RAS, 142432 Chernogolovka, Russia Abstract From experiments with amorphous InO lms, three conclusions are made: (i) The pattern of the superconducV tor}insulator transition (SIT) seen before for 2D ... Fig. ... Hence, in each "eld the bosons and the fermions coexist. ...

We present a detailed study of how the star formation rate (SFR) relates to the interstellar medium (ISM) of M31 at ~140 pc scales. ... The relationship between SFR and gas surface density is tested in six radial annuli across M31, assuming a power law relationship with index, N. The star formation (SF) law using total gas traced by H I and CO gives a global index of N = 2.03 б± 0.04, with a significant variation with radius; the highest values are observed in the 10 kpc ring. ...

The very metal-poor local dwarf galaxies - the analogs of primordial galaxies in young Universe . ... The goal of this project is the study of the properties of the local eXtremely Metal-Deficient (XMD) dwarf galaxies. ... S.A. Pustilnik, J.-M. Martin . ... Pustilnik S.A. "Dark galaxies" and local very metal-poor gas-rich galaxies: possible interrelations, in: Dark Galaxies and Lost Baryons, Edited by J.Davies and M.Disney, Proceedings of IAU Symposium No. 244, held 25-30 June, 2007 in Cardiff, UK. ...

... Compressional Pc 5 ( ULF ) waves, found on the nightside close to the flanks of the magnetosphere , are the dominant pulsations occurring beyond L =8. ... Accordingly, the events are strongly associated with high beta plasma clouds and are much more likely to be observed near the equator than >10њ off the equator (see, e.g., Anderson, 1993). ... Azimuthally polarized toroidal Pc 5 pulsations are thought to be fundamental mode toroidal field line resonances (FLR) with magnetic node at the equator. ...

... Staff . ... Galaxies, AGN, Cosmology . ... Star formation . ... ALMA . ... A local window on galaxy formation with ALMA . ... Highly star-forming, metal-poor dwarf galaxies in the vicinity of the Milky Way offer an unique window over the conditions of primordial galaxy formation and evolution. ... The primary science goals of submillimeter astronomy with ALMA are: the high-redshift Universe and Cosmology, galaxies and AGNs, star formation and interstellar medium, exoplanets and stellar evolution. ...

Next: Back-End Signal Processors Up: The Arecibo Observatory and Previous: Available Receivers . All receivers at the Arecibo telescope use local oscillators locked to the station hydrogen maser frequency/time standard. Commercial synthesizers in the dome and carriage house are remotely controlled to provide the first LO. ... Next: Back-End Signal Processors Up: The Arecibo Observatory and Previous: Available Receivers Robert Minchin 2012-02-22 ...

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Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 05 - 11.08.2013, Forecast on 12 - 19.08.2013, Carrington Rotations 2140 (04,64.08.2013) SUNSPOT-FORMING ACTIVITY OF THE SUN REMAINED AT THE AVERAGE LEVEL, GRADUALLY INCREASING. ... FLARE ACTIVITY WAS AT THE VERY LOW LEVEL TO 9.08 AND THE LOW - IN OTHER DAYS. ... BY SOHO AND STEREO CORONOGRAPHS DATA THERE WERE OBSERVED 34 CME FROM WHICH 4 WERE THE "PARTIAL HALO II" TYPE. ...

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Here we present the ionospheric parameters variations for quiet conditions. ...

... We present a new technique to segregate old and young stellar populations in galactic spectra using machine learning methods. We used an ensemble of classifiers, each classifier in the ensemble specializes in young or old populations and was trained with locally weighted regression and tested using ten-fold cross-validation. ... In this work we propose a Machine Learning (ML) method to determine the age of stellar populations in synthetic galactic spectra. ...

I. Effects of local geometry on Accumulation and Desorption of ice Michael Hecht, Jet Propulsion Laboratory · · · · Importance of local geometry on a local scale Importance of local geometry on a global scale CO2 roughness and albedo H2O temperature variations & humidity HEND Workshop, June 9, 2003 1 Topography, Topography, Topography Several papers have addressed thermal balance of small 3-D structures on Mars (many have addressed slopes). ... For CO2 ice, water could be a factor. ...

Next: Morlet transform of Up: No Title Previous: Inverse transform . ... Figure 16: Real (solid line) and imaginary (dashed line) parts of the Morlet wavelet for . ... Clearly, the wavelet transform will have a real and an imaginary part, and it is useful to represent them in `polar' coordinates: the norm is the magnitude of the transform and, being related to the local energy, is of primary interest, while the polar angle (phase) completes the representation. ...

... For example, the invariants are in general closely related with the closed orbits, and the orbit of a representation V is closed if and only if V is semi-simple and in this case the slice ґ etale at V is described in terms of a local quiver V , which is defined from the indecomposable summands of V (see [LBP]). ... The condition (ii) of the Theorem allows to apply Luna ґ etale slice Theorem [Lu], and the slice at V is described by the local quiver V exactly in the same style as in semi-simple case. ...

... 24.09.2013 . ... A working map of the local ISM within 20 light-years, based on ongoing observations and recent particle detections from the Earth-orbiting Interstellar Boundary Exporer satellite ( IBEX ), is shown above . These observations indicate that our Sun is moving through a Local Interstellar Cloud as this cloud flows outwards from the Scorpius-Centaurus Association star forming region . Our Sun may exit the Local Cloud , also called the Local Fluff, during the next 10,000 years. ...