... MATHEMATICS Evaluation of Multiple Eigenvalues and Jordan Chains of Vectors for Matrices Depending on Parameters A. A. Mailybaev Presented by Academician N.S. Bakhvalov April 5, 2001 Received April 6, 2001 The reduction of a matrix to the Jordan form is an unstable operation if the matrix has multiple eigenvalues. ... Let p' d be a point in this manifold. ... The multiple eigenvalues and the corresponding Jordan chains at the points of stratum are defined by relations (6), (7) for every i' . ...

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• http://mailybaev.imec.msu.ru/papers/KuznetsovEtAl2008.pdf
• http://mailybaev.imec.msu.ru/papers/Mailybaev2005.pdf

... Real environments where objects are settled down are non-uniform and they are the source of many physical problems of acoustical imaging. ... Two groups of methods of image reconstruction in non-uniform environments are considered, and the basic attention is given to nonlinear phase methods as unlike methods of the first group, wave front inversion by matched filtering processing, they do not require detailed knowledge of parameters of the non-uniform medium. ... Acoustics of non-uniform mediums. ...

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ISSN 0026-8933, Molecular Biology, 2007, Vol. ... PROTEOMICS UDC 575.174:575.858:553.2 Molecular Genetic Diversification of the Lizard Complex Darevskia raddei (Sauria: Lacertidae): Early Stages of Speciation V. V. Grechkoa, A. A. Bannikovab, S. A. Kosushkina, N. L. Ryabininaa, K. D. Miltoc, I. S. Darevskyc, and D. A. Kramerova Engelhardt Institute of Molecular Biology, Russian Academy of Sciences, Moscow, 119991 Russia; e-mail: grechko@eimb.ru b Moscow State University, Moscow, 119992 Russia ...

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• Выступления студентов и аспирантов на конференциях
• Student Reports at International Conferences

... initial value of E in linear potential sweep voltammetry), was derived for reversible reaction O + ne R proceeding in a compact film adsorbed onto an electrode of surface A. A series of inferences from this equation, namely: (1) the appearance of peak current ip at potential value E = Ep (i.e. = 1); (2) the equality of adsorption densities of reduced (R) and oxidized forms (O) to each ... Case II: reaction on the film physical border (including lateral surface of pores). ...

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• http://www.elch.chem.msu.ru/mole/lecture/qavdeev.pdf

A&A 369, 965­970 (2001) DOI: 10.1051/0004-6361:20010159 c ESO 2001 Astronomy & Astrophysics Formation of Fe X­Fe XIV coronal lines in the accretion shock of T Tauri stars S. A. Lamzin1 , H. C. Stemp els2 , and N. E. Piskunov2 1 2 Sternberg Astronomical Institute, Moscow V-234, 119899 Russia e-mail: lamzin@sai.msu.ru Uppsala Astronomical Observatory, Box 515, 751 20 Uppsala, Sweden e-mail: stempels@astro.uu.se Received 26 October 2000 / Accepted 24 January 2001 Abstract. ... S. A. Lamzin et al.: ...

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• http://www.sai.msu.ru/dept/adm/lamzin/aa1179.pdf
• http://www.sai.msu.ru/dept/adm/lamzin/aa2787.pdf

Contents Curricula, and Programs. Mathematical Analysis. (The Program of Mathematical Physics Department).............................................. Algebra and Analytical Geometry.(The program of (General "Mathematics" Department)................................ Computer and Programming. (The program of Algorithmic Languages Department).................................... The practical work on Computers.( Department of Algorithmic. Languages)............................................... Discrete

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... In the light curve depicting their observations, definite trends are noted, here is a "thumb-nail" analysis of the the magnitude estimations of the bright SN (1989B) in the galaxy NGC 3627 (M66). ... 10 (IAUC # 4742) 2/25 13.3 16 j 2/27 13.5(*) 18 lc 2/28 13.8 19 p 3/1 13.2 20 w 3/2 13.5 21 a 3/4 13.8 23 p 3/6 13.3 25 c 3/7 13.3 26 c 3/8 14.1 27 m 3/8 13.3 27 r 3/9 13.4 28 c 3/9 14.1 28 m 3/10 13.6 29 j 3/10 14.0 29 a 3/11 13.6 30 c 3/11 13.5 30 r 3/11 13.7 30 s 3/13 [13.69 CCD Mag.] ...

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• THE BRIGHT SUPERNOVA 1991T IN NGC 4527; AN AMATEURS PRESPECTIVE
• Images of Supernova 1998S in NGC 3877
• Images of Supernova 1998aq in NGC 3982

... June 9, 1999 . NGC 4414: A Telling Spiral . ... the Hubble Heritage Team ( AURA / STScI / NASA ) . Explanation: How far away is this galaxy? ... Spiral galaxy NGC 4414 contains many Cepheid variable stars that oscillate in a way that allows astronomers to estimate their distance. ... NGC 4414 shows many classic spiral galaxy features, including thick dust lanes , a central region rich in old red stars, and winding spiral arms glowing with young blue stars. ... About APOD > . ...

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• APOD: April 2, 1999 - Stars of NGC 206
• APOD: 2000 March 12 - Supernova 1994D and the Unexpected Universe
• APOD: December 30, 1998 - Supernova 1994D and the Unexpected Universe

... Using the CFBDSIR wide field survey for brown dwarfs, we identified CFBDSIRJ214947.2-040308.9, a late T dwarf with atypically red J-Ks colour. ... SN 2009ip in NGC 7259 Electronic Telegram No. ... 7.09, [19.0; 2009 Aug. ... Accepted for publication in MNRAS Subjects: High Energy Astrophysical Phenomena (astro-ph.HE) The jet opening angle theta_jet and the bulk Lorentz factor Gamma_0 are crucial parameters for the computation of the energetics of Gamma Ray Bursts (GRBs). ...

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• http://master.sai.msu.ru/static/YaB_100/20/Khlopov.pdf
• SAI Space Monitoring Laboratory
• Ya.B. Zeldovich All-Moscow Seminar of Astrophysicists

... In general, the entire flow domain in the entry region of a channel can be split into five asymptotic domains Fig. 2 : 1 the region of a uniform free stream, where the parameters are the same as in the inlet section the fluid velocity and particle concentration profiles are uniform and the particle slip velocity is zero , 2 the boundary layer on the channel wall, where the fluid velocity profile is nonuniform, ... The particle concentration is found from explicit formula 22 ....

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• http://new.math.msu.su/department/hydro/papers/Asmolov-Osiptsov-paper-PoF-2009.pdf
• http://new.math.msu.su/department/hydro/papers/gol-dor-leo-2009.pdf
• http://new.math.msu.su/department/hydro/papers/2012-jfs.pdf

... For full UV energy Euv (erg) radiated in TLE the corresponding number of photons of wavelength =300-400 nm (with average energy 3.5 eV) is: Nph=Euv/3.5в1.6 10-12 (1) We considered 2 options of the pinhole camera focal distance: 1. focal distance is short so that the circle of diameter 40 km is observed by one pixel and 2. focal distance is long so that the 40 km circle is observed in many camera pixels. ... Full energy released in UV in the atmosphere is determined by the pixel signal. ...

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• http://cosrad.sinp.msu.ru/experiments/tus/doc/HO2COSPAR2006.pdf

... 'objectif du programme est triple: - observer comment le confessionnel, l'ethnique et le protonational contribuaient Ю la construc