... arXiv.org . astro-ph . ... We fit the near-infrared to radio spectral energy distributions of 30 luminous and ultra-luminous infrared galaxies with pure starburst models or models that include both starburst and AGN components to determine important physical parameters for this population of objects. In particular we constrain the optical depth towards the luminosity source, the star formation rate, the star formation efficiency and the AGN fraction. ...

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... Research objects and scientific purposes . Space scientific program includes development and launch of two supersmall spacecrafts "Universitetskiy" and "Kompas-2" intended for monitoring of radiation conditions near the Earth. ... All the studies conducted in the near-Earth space are characterised by strong radiation fields. ... The circular polar orbits, which cover all the near-Earth space, are the most favorable for comprehensive studies of the radiation conditions near the Earth. ...

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... Центральное место в курсе занимает комплекс асимптотических результатов теории вероятностей, включающий, наряду с законом больших чисел и классической центральной предельной теоремой, обобщение последней для устойчивых законов и теоремы о предельных распределениях экстремальных значений и больших уклонений. ... Теория распределений . ... Причина нарушения закона больших чисел для распределений с тяжелыми хвостами , статистика экстремальных значений, предельная теорема Фишера-Типпета-Гнеденко. ...

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• IUM (Spring 2014)
• Mathematical statistics: an introduction (Fall 2011)
• Labo J.-V.Poncelet: G.Koshevoy

... Bojan Nikolic web pages (r. 329) . Lectures and related materials . Lecture 1 handout . ... Mike Irwin?s lectures: http://www.ast.cam.ac.uk/~mike/lect.html . Penn Astro-Statistics pages: http://astrostatistics.psu.edu/ . Steve Gull?s page on Bayesian radio-astronomy: http://www.mrao.cam.ac.uk/~steve/algor2008/index.html . ... Statistics for astronomy graduate course . ... Astrophysical techniques graduate course . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

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• OptInt PmWiki : MROIFastTipTilt / Tech Meet 1
• Statistics for astronomy graduate course
• OptInt PmWiki : Tech Meet 1 | History

Life from Mars: . The Discovery . ... Meteorite Yields Evidence of Primitive Life on Early Mars (August 7, 1996) . Life from Mars: Video Animations . ... The NASA-funded team found the first organic molecules thought to be of Martian origin; several mineral features characteristic of biological activity; and possible microscopic fossils of primitive, bacteria-like organisms inside of an ancient Martian rock that fell to Earth as a meteorite. ... Mars Life? Microscopic Structures . ...

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• mod_status - Apache HTTP Server
• Comet Halley
• Arcetri Solar Physics Group: Solar Activity

... Accordingly, every accumulation carries extra total, which readily adjusted off­line subtracting number clock cycles integration from readout value of accumulation (taking care remember least significant bits resident Two and Three­level digitization digitizer samples the instantaneous input voltage rates 100 MHz. ... Multibit Sampling lags) the multibit case, scatter zero (Power) given by “ “ m ) / m 2 where m represents multibit N number samples used form estimate. ...

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• http://www.naic.edu/~phil/rfi/gps/l2c_presentation.pdf
• http://www.naic.edu/~tghosh/PP-LRP.jul97
• pdev_birdies_25jun07

. My astronomical research interests center on galaxy structure and evolution. Current topics include: . Polar-ring and interacting galaxies (see also new catalogue ) . Galaxy warps: statistics, properties and origin . Spiral galaxies at z~1: radial and vertical structure of stellar disks, statistics of interactions . Surface photometry and kinematics, dynamical modeling . Observational cosmology . Joomla Counter since Sep 1997

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• Linear polarization: wavelength dependence

... The Sun is the closest star to us, and a regular object in our Galaxy. Solar activity manifests itself, primarily, in solar flares - episodic explosive energy release in the form of electromagnetic radiation and high energy particles (electrons and protons). The nature of the flares is related to cyclic variations of global and local magnetic fields in the atmosphere of the Sun. ... Such formations are called active regions. ...

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• Detection of polarized radiation sources with unusual spectral characteristics
• Detection of unique bright radio flare of X-ray binary

This module provides information on server activity and performance. ... Compatibility: Available in Apache 1.1 and later. ... ExtendedStatus To enable status reports only for browsers from the foo.com domain add this code to your httpd.conf configuration file <Location /server-status> SetHandler server-status Order Deny,Allow Deny from all Allow from .foo.com </Location> . ... A machine-readable version of the status file is available by accessing the page http://your.server.name/server-status?auto . ...

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• Log Files - Apache HTTP Server

.

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• RSAA Honours Courses (2006)
• Siding Spring Survey 2004 CB
• C/2006 P1 (McNaught)

... Other Characteristics of the Sun: Variability of Rotation, Magnetism, Chemical Structure, Planetary System. ... Methods of Solar Magnetic Fields Measuring: Visual, Photografic, Photoelectric. ... Empiric Datas of Magnetic Fields in Photosphere, Chromosphere and Corona. ... Characteristics of Magnetic Field in Balanced Force Tubes by Potential and Forceless Field. ... Phenomenons in Active Region (Magnetic Field, Spots, Torches, Solar Prominences, Flares, Discharges. ... Magnetic Fields in Flares. ...

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• WARNING MISSION: Background
• Stellar Astronomy
• Solar-Terrestrial Connections

... IONOSPHERIC DATA IN THE INTERACTIVE SPIDR SYSTEM . ... The Ionosphere The ionosphere is that part of the upper atmosphere where free electrons occur in sufficient density to have an appreciable influence on the propagation of radio frequency electromagnetic waves. ... These regions may be further divided into several regularly occurring layers, such as F1 or F2. ... E Region: The region between about 95 and 150km above the Earth that marks the height of the regular daytime E layer. ...

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• http://www.wdcb.ru/stp/data/geomagni.ind/kp_ap/apstar/ReadmeAPSTAR
• http://www.wdcb.ru/stp/data/geomagni.ind/aa/aastar/aastar_readme.htm
• http://www.wdcb.ru/stp/data/geomagni.ind/kp_ap/11Kp_Ap_fmt.txt

... ON THE ROLE OF LARGE-SCALE PLASMA IRREGULARITIES AT THE FINAL STAGE OF ANOMALOUS ABSOPTION DEVELOPING UNDER HF HEATING OF THE IONOSPHERE . ... Fig. ... With the aid of numerical statistical modeling based on multiple ray tracing it is shown that in presence of large-scale irregularities the reflected signal amplitude mean value is increased significantly. ... Dependence of the mean amplitude of the reflected from the ionosphere signal on the large-scale (10-50 km) electron density irregularity level...

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• V.Marsakov, Yu.Shevelev, F-stars in galactic disk

... For every level we have plotted the dependence between width and Lande factor and obtained the linear regression parameters: the inclination, the zero Lande factor line width and the correlation. ... Fig. 1. presents a model components, the intensity of which decreases (b) line with 10 and increases (c) to the center of spectral line (the field is 12 k6s). ... Our results show strong dependencies of line width on the level of width measurements. ...

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• http://mavr.sao.ru/hq/lizm/conferences/pdf/2003/2003_p19.pdf
• Description of algorithm
• Experimetn COLD: Introduction

... ClassљIndex . ... StelRendererStatistics Class Reference . Stores and provides access to statistics about a StelRenderer backend. ... getNext (const char *&name, double &value) . Get next statistic name and value. ... Access statistic with specified index to modify it. ... while (statistics.getNext(name, value)) . ... Name of the statistic will be stored here (only a pointer to it). value . ... A clean way to do this is to use an enum with name corresponding to the name of the statistic. ...

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• AWStats (unofficial version)
• Stellarium: RendererStatistics Class Reference
• Stellarium: core/renderer/StelRendererStatistics.hpp Source File

Dynamics and Statistics M/M 10 4 statistics R = 0.9992 2 103 dynamics R = 0.9401 10 2 2 log(/o) -1.8 -1.7 -1.6 -1.5 -1.4 -1.3 -1.2 -1.1 -1 Comparison of results of mass estimation which is received by means of our method (dynamics) for 18 clusters of Milky Way with suspected BH with data in [2] (Safonova, Shastri, Aph. ... We considered the limits of central bodies masses for 4 clusters in our Galaxy (47 Tuc, Cen, NGC 6388, M15) and G1 Globular cluster in the Galaxy Andromeda. ...

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... the total number of numbered minor planets is 350441 ; . the total number of named minor planets is 17621 ; . the unnamed minor planet with the least number: (3708) 1974 FV1 ; . the named minor planet with the greatest number: (340980) Bad Vilbel ; . the total number of minor planet names containing symbols with diacritical characters is 839 ; . ... the first minor planet named using a symbol with diacritical character is (61) Dana?. ... Symbol . ... Minor planet names ...

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• Conference WPLTN-2012 | Conference page
• IAA VLBI Analysis Center
• (Untitled)

RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . ... SSRT - Possibilities of observing . ... Investigations of the SSRT 5.7 GHz radio maps in conjunction with images obtained in other emission ranges, suggested the following conclsions: . ... Solar images obtained in line H a ;(on the left, 16:11 UT, Big Bear observatory) and in the microwave emission (on the right, 04:04 UT, SSRT) 4 march 1997 . ...

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... Мир 1979. ... А.Б.Шмидт , Статистическая термодинамика классической плазмы, М., Энергоатомиздат, 1991. ... Кайзер , Статистическая термодинамика неравновесных процессов. ... И.П.Базаров, Э.В.Геворкян, П.Н.Николаев , Задачи по термодинамике и статистической физике. ... Ю.Б.Румер, М.Ш.Рывкин , Термодинамика статистическая физика и кинетика, М., Наука, 1972. ( pdf-pages ) . ... А.Исихара , Статистическая физика, Мир, 1973 (см. pdf ) . Термодинамика и статистическая физика, РХД, CD . ...

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• Work notes
• Perfect gas - statistics
• Coaxial jets

GCVS Variability Types and Distribution Statistics of Designated Variable Stars According to their Types of Variability ======================================================================== I. GCVS Variability Types. ... Amplitudes usually do not exceed 0.1 mag. ... RR Variables of the RR Lyrae type, which are radially-pulsating giant A-F stars having amplitudes from 0.2 to 2 mag in V. Cases of variable light-curve shapes as well as variable periods are known. ... RV Variables of the RV Tauri type. ...

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• General Catalogue of Variable Stars: Variability Types