... We proposed that information retrieved from the local surface photometric behavior of the Moon could be used for guiding the remote sensing analyses of specific geological targets. ... The value of the difference of intensities mentioned above may be used as a photometric parameter I of the local surface roughness. ... 7] Apollo 11 Prelim. ... Figure 5 represents the diagram of relationship between photometric roughness parameter and local thorium content in different lunar regions. ...

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• http://selena.sai.msu.ru/Rod/Publications/ms40/78_Sitnikov_etal.pdf
• http://selena.sai.msu.ru/Shev/Publications/ms38/ms083.pdf
• http://selena.sai.msu.ru/Shev/Publications/m44_76_sinitsin_shevchenko.pdf

The software available here is only available on an "as-is" basis. ... If you use this software, and it breaks your camera it is not my fault. First, there was QVplay . ... My first qv-300 webcam used this software, and a perl script that I put together. ... Note that the perl script had to be set up to copy the file to the web server, because NFS can't be trusted to update file modification times in a timely fashion. ... Beau software also sells webcam software for the QV cameras. ...

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• The AstroStat Slog Blog Archive chi-square distribution [Eqn]
• The AstroStat Slog Blog Archive tests of fit for the Poisson distribution
• Comments on: chi-square distribution [Eqn] By: Alex By: vlk By: aneta By: aneta

... 13-Aug-2014 12:13 106K lk_20140815_0905.tar.. 15-Aug-2014 09:06 106K lk_20140901_0823.tar.. 01-Sep-2014 08:23 103K lk_20141016_1324.tar.. 16-Oct-2014 13:25 103K lk_20141211_1708.tar.. 11-Dec-2014 17:08 103K lk_20150430_0315.tar.. 30-Apr-2015 03:15 103K lk_20150430_0420.tar.. 30-Apr-2015 04:20 103K lk_20150818_1511.tar.. 18-Aug-2015 15:11 104K lk_20151113_1903.tar.. 13-Nov-2015 19:04 105K lk_20160314_0610.tar.. 14-Mar-2016 06:11 105K . ...

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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. ...

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• Extragalactic Astronomy
• INFRARED FOURIER-SPECTROMETER SICH-F

... The distribution of redshifts among the DXRBS FSRQs identified so far (Figure 3) is quite similar to that of the 1 Jy and S4 samples. ... A more thorough comparison will have to await completion of our survey and the convolution of the redshift distribution with the WGACAT sky coverage. As has already been mentioned by Hook et al. (1996), selecting flat-spectrum sources is an efficient way of finding high-redshift, radio-loud quasars. ...

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• ESO - ESO-MIDAS Releases and Distribution
• ESO - European ALMA Regional Centre
• IAU Symp317 Scientific Program

spaceweb@oulu.fi - last update: 1 July 1998, 1200 UT (RR) . ... Relates the wave number k to the wave frequency. ... From the equation of motion , m d v /dt = q( v x B ) one can calculate that, in a presence of magnetic field B , a charged particle is accelerated in direction perpendicular to both v (perp) and B . ... The angle a between magnetic field B and velocity vector of a charged particle, v ., i.e., sin a = v(perp) / v(total), where v(perp) refers to the velocity component perpendicular to B . ...

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Distribution of the analyzed SEPs with different >100 MeV proton fluxes ( J 100 ) at the microwave flux density plane ' S 9 vs. ... 1) General correspondence takes place between intensities of microwave bursts and proton fluxes - J 100 increases when S 9 and S 15 rise. ... 3) Powerful microwave bursts ( S 9 , S 15 >3000-10000 sfu ) with hard radio spectra ( S 9 < S 15 ) correspond to majority of powerful proton fluxes ( J 100 >10 pfu ). ...

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• Space weather and ecology
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• Publications for 1995-1999

... М.С.Агранович об опыте чтения лекций в НМУ, апрель 2009. В 2002-2007 гг. я прочитал в НМУ несколько спецкурсов по анализу: "Обобщенные функции", "Соболевские пространства", "Эллиптические псевдодифференциальные операторы" (общая теория и элементы спектральной теории), "Несамосопряженные операторы". ... Эллиптические псевдодифференциальные операторы", . Операторы с дискретным спектром" . ... Лекция 1 (48K) | ... Структура обобщенных функций из пространств $\Cal S'$ и $\Cal E'$. ...

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• Young researchers' seminar in statistical physics
• Distributions and Sobolev spaces (Fall 2005)
• Dubna-2003: Diagonoal method; distribution of primes

. Vendor contact information . Bastille Linux . Caldera . Debian . Kha0s . NetMAX . Red Hat . Slackware . Stormix . SuSE . TurboLinux . Back . Written by Kurt Seifried

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• research field
• LASG - Secure Linux distributions
• Arcetri Open Time

. Fractal Matter Distribution . Observed fractal galaxy distribution is discuused in: . F.Sylos Labini, M.Montuori L.Pietronero, "Scale invariance of galaxy clustering" astro-ph/9711073 . The home page of "The Debate on fractal Universe"

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• Local Group Dynamics
• The Local Group
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. Name . Last Modified . Size . Type . Parent Directory / . - . Directory . 10.2 / . 2009-Dec-06 17:59:27 . - . Directory . lighttpd/1.4.37

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... Results 3. ... 2004), Escapa (2011): Hamiltonian approach, simplified elastic response. ... PАg. ... Let us recall that assuming a rheological model based in Smith (1974) , Wahr (1979) and IERS (2010) for the elastic/anelastic response of the Earth, the second order harmonic components of the redistribution potential admit a truncated development in complex spherical harmonics in the form Generalized Love Numbers, dependent on: Harmonic order, Excitation frequencies In magnitude, PАg. ...

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• Страница Е.В.Милецкого / Page of Eugen Miletsky
• Local Organizing Committee:
• Бобылев Вадим Вадимович

To construct two-dimension distribution of minor planets user should specify elements/ parameters/ function that will be plotted as abscissas and ordinates. In three-dimension case one should add to them the element plotted on Z axis. ... Though you may choose elements plotted along different axes at will, often there is good reason to plot such elements as a, n, or n" along X axis (two-dimension distributions) and to plot them along Y axis in three-dimension case. ...

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• Keywords_120
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. Red histogram is 2dF QSO Redshift Survey . Blue histogram is Durham/AAT QSO Survey . | Front page | . | << - Number Counts | . Robert J. Smith, ">rsmith@mso.anu.edu.au Last modified: Fri Sep 24 11:39:02 EST 1999 .

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... Local organizer: Dr. Mikhail Sosonkin, Main Astronomical Observatory, Ukrainian National Academy of Science (NAS of Ukraine), Kiev . ... Leader of the group "ozone research" at the Institute for Atmospheric and Climate (IACETH), Swiss Federal Institute of Technology Zurich (ETHZ), Switzerland . ... Head of Laboratory for Atmosphere Optics, Main Astronomical Observatory, Ukrainian National Academy of Science (NAS of Ukraine), Kiev . ... Coffee break (10.45-11.15) . ... Coffee Break (14.30-14.50) . ...

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• Olga V. Zakhozhay
• Administration

... The obtained results lead to the following conclusions: a) the heavy element enrichment had taken place in the Galaxy in a few bursts of its activity rether than in a continuons manner; b) these bursts occured during the callapse of the early Galaxy; c) the star formation had been inhibited in the time of the bursts; d) the metal enrichment did not proceed in the periods of star formation, between these bursts of activity. ...

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• RR LYRAE VARIABLES SUBSYSTEMS IN THE GALAXY, figures
• MONTE-CARLO
• Vladimir Marsakov Publication List

... Parallel Tree N­body Code: Data Distribution and DLB on the CRAY T3D for Large Simulations U. Becciani, V. Antonuccio­Delogu, M. Gambera and A. Pagliaro Osservatorio Astrofisico di Catania, Citt‘a Universitaria, Viale A. Doria, 6 -- I­95125 Catania ­ Italy R. Ansaloni Silicon Graphics S.p.A. St.6 Pal. ... A bodies data distribution ranging from contiguous blocks (coarse grain: cdir$ shared pos(:block,:)) to a fine grain distribution (tf) (cdir$ shared pos(:block(1),:)) was adopted. ...

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• http://www.stecf.org/conferences/adass/adassVII/reprints/daszynskaj.ps.gz
• http://www.stecf.org/conferences/adass/adassVII/reprints/nishiharae.ps.gz

Copyright (c) 2014, 2015>, University of Washington All rights reserved. Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. ... THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. ...

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• Astrophysical Research Consortium - Apache Point Observatory
• Hipparcos Tycho catalog
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... Email: chaos@mail.cplire.ru . ... In this report, we investigate phenomena on the edge of spatially uniform chaotic mode and spatial temporal chaos in a lattice of chaotic 1-D maps with only local connections. It is shown that in autonomous lattice with local connections, spatially uniform chaotic mode cannot exist if the Lyapunov exponent of the isolated chaotic map is greater than some critical value cr > 0. ...

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• Edge of Spatial Chaos in Nonlinear Networks with Local Connections - CNNA-98
• Conditions for Global Synchronization - Bif. and Chaos
• Lab 234 - SQUID amplifier

. 2 klasa, osobowy 2 klasa, pospieszny 1 klasa, pospieszny . PARAVOZ (Page of Dmitry ZINOVIEV) Local mirror . INTERNATIONAL Union of Railways . Passenger Moscow Service... Public Moscow transport... Moscow Tram .

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• http://lnfm1.sai.msu.ru/~rastor/Ralf_Bender/imprs_chapter_11_2007_dwarf_galaxies.pdf
• http://lnfm1.sai.msu.ru/~rastor/Ralf_Bender/imprs_chapter_13_2007_large_scale_structure.pdf