... The internal thermal fields in non-rotating spheroidal particles illuminated by intense laser pulse were considered by Astafieva & Babenko ("Heating of a spheroidal particle by intense laser radiation." ... Ocean Optics, v. 11, 1, 1998), Astafieva & Babenko ("Heating of a spheroidal particle by intense laser radiation." ... Kokhanovsky A.A. (1999) Optics of Light Scattering Media. ... 4.10.Astafieva L.G., Babenko V.A. (1999) Heating of a spheroidal particle by intense laser radiation. ...

... Posts tagged ?posterior distribution? ... stat.AP:0811.1663] . Open Statistical Issues in Particle Physics by Louis Lyons . ... Category: arXiv , Bayesian , Cross-Cultural , Data Processing , Frequentist , High-Energy , Methods , Physics , Stat | ... Accounting for Spatial Correlation in the Scan Statistic by Loh &Zhu [stat.AP:0712.1458] provides a picture that helps us to understand excessive false alarms in source detection when the image data set is based on the Poisson point process. ...

EXPERIMENT . ... Charged energetic particles (Ee=40-200 keV; Ei=0.05-150 keV) composition and anisotropy. ... IKI, Moscow, Russia . ... University of Thrace, Xanthi, Greece . ... Energy spectra, angular distributions and time variations of electrons (E=15-400 keV) and ions (E=20-1000 keV). ... IMBP, Moscow, Russia . ... Moscow University, Moscow, Russia . ... IPG, Moscow, Russia . ...

Next: Abstract . Mikhail E. Prokhorov and Konstantin A. Postnov . ... Physics of Neutron Stars'' . ... Abstract . ... Initial conditions . Space and velocity distributions . Space position . Initial velocity . ... Mike E. Prokhorov . ...

... The MIDAS system is available, free of charge, to all non--profit research institutes, whereas other organisations or companies may be charged a nominal fee to cover distribution. Institutes interested in using MIDAS must sign a User Agreement before they receive MIDAS. The necessary forms can be obtained by contacting the Data Analysis Group at ESO/Munich. ... The current system at ESO/Munich is frozen several months prior to the official release. ...

... Abstract . ... GRB afterglows and host galaxies at very high redshifts . ... The cosmic distance scale and dark energy are two key issues in modern astrophysics, and HST has played a vital role in probing both. ... The Sloan sky survey provides a powerful tool for identifying candidate galaxy-galaxy lenses; this program is using HST-ACS imaging to verify the nature of those candidates, and provide the angular resolution necessary to model the mass distribution. Past weeks: . ...

ENERGETIC PARTICLE EXPERIMENT DOK-2 . ... Due to much higher energy, angular and time resolution, better separation of electrons and ions it is expected that DOK-2 experiment will allow to re-examine in more details energetic particle population and related processes in magnetosphere regions covered by the spacecraft orbit. ... Thin foil in front of detector absorbes protons with energies E<400 keV so this detector measures electron spectrum in 20 - 420 keV range. ... Energy values, keV . ...

FEATURES OF THE HYDROGEN DISTRIBUTION AROUND LUNAR CRATERS PROCLUS AND KEPLER. ... In result of analysis of the data Lawrence and Feldman constructed the hydrogen distribution on the lunar surface [1]. ... However, the authors shown, that EN flux data features may be explained by other element abundance in the lunar soils, namely: Si, Ca, Gadolinium (Gd), Samarium (Sm) and Fe. ... Using of the Feldman's interpretation of the Lunar Prospector data [8], we constructed hydrogen distribution map (Fig.1). ...

... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...

... к почтовому серверу ГАИШ lnfm1.sai.msu.ru . ... WEB-страницы отделов ГАИШ . ... на LNFM1 . HERITAGE - АСТРОНОМИЧЕСКОЕ НАСЛЕДИЕ . астрономическое образование с сохранением традиций) . Лаборатория Новых Фотометрических Методов . ... Леонтьев Сергей Ефимович . ... Копаев Александр А. Отдел Радиоастрономии . Татарников Андрей М. Пахомов Юрий . ... Гусев Александр Сергеевич . ... Кононович Эдвард В. Купряков Юрий А. Горшков Алексей Б. Отдел Звездной астрофизики . ... Моисеев Алексей . ...

... Modern aspects of statistical physics and its applications. The seminar welcomes survey talks by senior researchers for the student audience and, more importantly, talks by students of undergraduate and graduate level on their research in progress. ... Olga STETIUKHINA, MSU Math. ... Anna BODROVA, MSU Physics Dept : Size distribution of particles in the rings of Saturn . ... Misha TAMM, MSU Physics Dept : A queue model (continued) . ... Misha TAMM, MSU Physics Dept : A queue model . ...

... Dept. for Physics of Stars&Galaxies . ... Astronomical Calendar . ... History of MAO . ... БЂ“ 2013. ... Zakhozhay O. and Vorobyov E.I. The signatures of disk fragmentation in spectral energy distributions // Proceedings of the conference Hot Planets and Cool Stars, Garching, November 12-16, 2012. ... Zakhozhay O.V., Vorobyov E.I. Spectral energy distributions of fragmenting protostellar disks // Formation, detection, and characterization of extrasolar habitable planets Proceedings IAU Symposium No....

... Effects of meteor ablation and the chemistry and physics of the upper atmosphere . ... Ablation and Ionization Modeling: Implications for Trail Instabilitiesand Head Echoes . Radar Observations of Meteors at a Polar Latitude . ... Radar meteor shower observations: processing and some results . ... Parameter estimation of meteors from radar head echoes combined with optical observations . ... Observations of meteor-head echoes using the Jicamarca 50 MHz radar in interferometer mode . ...

Imaging photometry of the optical continuum during Deep Impact Tanyu Bonev1 and Klaus Jockers Max Planck Institute fЭr Aeronomie · Feasibility · Brightness and color measurements of a disintegrated comet · Simulations of the impact ejecta dust cloud · Conclusions 1 on leave from I nsti tute of Astronomi e, Bulgari an Aca demy of Sc i ence s Feasibility or · What we know about the dust coma of comet 9P/Tempel? and · Is the material added by the impact sufficient to be detected? ...