... Rapid developments of lasers and particle accelerators resulted in implementation of laser plasma X-ray sources and free electron lasers for various experiments requiring high intensity, shrt duration and monochromatic X-ray radiation. ... BASICS AND APPROACH Thirty years development of laboratory X-ray lasers allowed to reach ~0.1 keV photon energy of coherent X-ray beams in a repetitive mode. ... X-rays originate from Thomson scattering of counter propagating laser and electron beams. ...
SUNY-MSU Partnership . ... MSU | ... The State University of New York/Moscow State University partnership dates back to the mid-1970s and owes its existence to the vision of then MSU Rektor Rem Kokhlov and SUNY Chancellor Ernest L. Boyer. ... The first students were exchanged in 1977. ... A SUNY Center on Russia and the United States opened its doors in January 2000, and a sister MSU Center on the United States and Russia was set up in Moscow at MSU?s newly built Science Park. ... suny-msu . ...
Переход на сайт учебного центра ЦНИР . ... О центре . ... С 3 по 8 февраля 2014 года в Объединенном институте ядерных исследований в г. Дубна будет проходить XXI Международная конференция ?Математика. Компьютер. ... Организаторами конференции являются Центр национального интеллектуального резерва МГУ, Фонд ?Национальное интеллектуальное развитие?, ... 2012 Центр национального интеллектуального резерва МГУ имени М.В. Ломоносова . ...
... DRIVER: Numerical simulation of transitional processes and features of developed turbulent regimes in flows of electrolytic solutions under electric field. ... DRIVER: Develpment of numerical modelling of noise generation processes in turbulent flows (jets, wakes, fans etc.) ... OBJECTIVE: As a result of numerical modelling, aerodynamic (mean parameters profiles, TKE distributions) and aeroacoustic (far field spectra) characteristics should be obtained for turbulent flows considered . ...
INNER POLAR RINGS REGULAR LENTICULAR GALAXIES 1 K. Sil'chenko 2 Sternberg Astronomical Institute, 119992 Moscow, Russia; Isaac Newton Institute Chile, Moscow Branch; olga@sai.msu.su Afanasiev Special Astrophysical Observatory, 369167 Nizhnij Arkhyz, Russia; vafan@sao.ru Received 2003 December accepted February 4 ABSTRACT have investigated a sample of galaxies, mostly with circumnuclear dust lanes orthogonal their major axes, chosen from Hubble Space Telescope Wide Field Planetary Camera 2 images. ...
... Школа по физике высоких энергий и ускорительной физике в CERN. Студенты кафедры физики ускорителей и радиационной медицины побывали на стажировке в ежегодной Школе по физике высоких энергий и ускорительной физике в CERN (г. Женева) с 5 сентября по 12 сентября 2014 года. ... И так, 18 июля 2014 в CERN (Женева) состоялось подведение итогов конкурса на участие в совместной ЦНИР МГУ - ОИЯИ - CERN Международной школе по физике высоких энергий и ускорительной физике. ... Введение в CERN. ... По CERN? ...
Network Working Group R. Fielding Request for Comments: 2068 UC Irvine Category: Standards Track J. Gettys J. Mogul DEC H. Frystyk T. Berners-Lee MIT/LCS January 1997 Hypertext Transfer Protocol -- HTTP/1.1 Status of this Memo This document specifies an Internet standards track protocol for the Internet community, and requests discussion and suggestions for improvements. Please refer to the current edition of the "Internet Official Protocol Standards" (STD 1) for the standardization state and status of this
... This sp ectral distribution is defined b oth by the energy distribution in the target star's sp ectrum and by the sp ectral resp onse of the detector, i.e. by the central wavelength 0 and the effective sp ectral bandwidth . ... On the right: The collection of the MASS sp ectral resp onse curves. ... Table 1: Integral characteristics of the resp onse curves of the MASS devices. 0 -- central wavelength, ef f -- effective wavelength for A0 V stars, -- effective bandwidth (integral under the curve). ...
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Ссылки http://curl.sai.msu.ru/mass/download/doc/mass_spectral_band_eng.pdf -- 303.9 Кб -- 15.12.2006 Похожие документы
... The data on UV glow of the atmosphere obtained in operation of one pixel of the TUS detector on board the Moscow State University "Universitetsky-Tatiana" satellite was taken into account in design of the updated TUS detector. ... The main feature of the design is use of MEMS technology scanning mirror controlled by the TUS computer, analyzing the recorded EAS data and directing the laser to the atmosphere spot, where back scattered Cherenkov light came from. ... Monitoring of UV intensity on-route....
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Ссылки http://cosrad.sinp.msu.ru/experiments/tus/doc/HO2COSPAR2006.pdf -- 237.2 Кб -- 19.03.2008 Похожие документы