PERFORMANCE COMPARISION OF KODAK DCS460 DIGITAL CAMERA AND PIXELVISION BACK-ILLUMINATED CCD . ... ABSTRACT : A Kodak DCS460 digital camera (with 1300 x 1000, 9-micron square pixels) and a PixelVision, back-illuminated digital CCD camera (with 1024 x 1024 elements, 12-micron square pixels) were tested at calibrated light levels ranging from 10 -2 footcandles to 10 -5 footcandles. The PixelVision back-illuminated CCD was shown to be 10,000 more sensitive than the Kodak DCS460 CCD camera. ...

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• Line Detection in the Comparison Spectrum
• Accuracy of data, comparison with independent measurements
• Comparison using a multiresolution quality criterion

... Информация Руководство и преподаватели Шахов Валентин Гаврилович . ... Публикации . ... Шахов В.Г. , Куркин Е.И. , Ляскин А.С. Расчет турбулентного течения во вращающемся диффузоре на основе вихреразрешающего подхода // Известия СНЦ РАН. 2013. ?6(3), т.15. ... Шахов В.Г. , Куркин Е.И. Модель турбулентности k-e в задаче пограничного слоя на вращающихся телах // Известия СНЦ РАН. 2012. ?4, т. 14. ... Ивченко А.В. , Журавлев О.А., Шахов В.Г. Газоразрядная генерация пристеночных течений // Вестник СГАУ....

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... We present an extensive comparison between the data and results obtained from the MAPPINGS II shock ionization code, and show that the physical properties of the line-emitting gas, including its ionization, excitation, dynamics and overall energy budget, are entirely consistent with a scenario involving auto-ionizing shocks as the dominant ionization mechanism. ... 2 ) ANU Astrophysical Theory Centre, Australian National University Canberra, ACT 0200, Australia 3 . ... huizinga@stsci.edu . ...

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• Comparisons Between Observed and Model PSFs in WFPC Image . Restoration
• Comparisons of Implementations
• A spatially resolved study of photoelectric heating and [C II] cooling in the

... A Statistical Comparison of Line Strength Variations in Coma and Cluster Galaxies at z 0.3 . ... We present a statistical comparison between spectral line strength variations in Coma galaxies and galaxies in three rich clusters at z 0.3. ... First, more independent parameters are required to account for the line strength variations in the distant cluster data than in the Coma data, and second, line strengths which are not correlated in the distant cluster data are strongly coupled in the Coma data. ...

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• SEST -- MOPRA Comparison at Millimetre-Waves
• Comparison with COBE
• difx:difx-sfxc_comparison [ATNF VLBI Wiki]

... MIPT Solid State Physics Department . ... Interacting Electrons in Normal Metals . ... The course is an introduction to interacting Fermi-particle physics and intended for future experimentalists. ... Hartree-Fock approximation. ... Linear reaction function. Calculation of density-density reaction function. Relation of density-density reaction function to compressibility of Fermi liquid and thermodynamic state density. ... Density-density reaction function of free Fermi gas in long-wave limit. ...

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• Department of Solid State Physics MIPT

... Flux density at 1 GHz (/Jy): 210 . ... Optical: Large filamentary loop, brightest to the NE, not well defined to the S or W. X-ray: Shell in soft X-rays. ... DRAO at 408 MHz (3'.3?6'.7) for spectral index study, plus X-ray and optical. ADS . ... Optical spectroscopy of nearside filaments. ... 1992, ApJ, 400, 214. ... IRAS observations. ... Leahy et al. ... Far-UV spectroscopy, H and other optical observations of NE region. ... Suzaku observations of NE. ... Suzaku observations of N. ADS . ...

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• Bojan Nikolic -- Fitting and Comparison of Models of Radio Spectra

... Empirical and theoretical modeling of 3-D structures in the solar corona is confronted by the tremendous amount of data needed to represent phenomena with a large dynamic range both in size and magnitude, and with a rapid temporal evolution. Octree representation of the 3-D coronal electron distribution offers the right compromise between resolution and size, allowing computation of synthetic images of the solar corona. ... The time interval between images is one day. ...

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• ADASS 2002 Conference Proceedings
• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
• Positive Iterative Deconvolution in Comparison to Richardson-Lucy Like

ALFA Pulsar Surveys Jim Cordes, Cornell University GALFA Workshop, Arecibo 20 March 2003 . ... Why more pulsars? Targeted Classes of Pulsars . ALFA Pulsar Surveys . ... Nominal Parameters of Galactic Plane Survey . ... Intermediate Latitude Survey . ... Issues for Optimizing Surveys . Pulsar Consortium Working Groups . ...

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• Pleiades VLA Survey Area Comparisons
• Comparison of AO, GBT & Parkes (Smin1 held fixed)
• Comparison of AO, GBT & Parkes Smin1 (AO) << Smin1 (Parkes)

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 large magnetic cloud caused by coronal mass ejection at the Sun on January 6, 1997 came to the Earth at early morning on January 10 and continue to interact with Earth's magnetosphere till January 11 (see for example home page of this event prepeared by Dr. M.Peredo http://www-istp.gsfc.nasa.gov/istp/cloud_jan97/event.html ). ... During the days discussed here INTERBALL-1 satellite was in the magnetosphere (MS) near its dusk flunk - see the Fig. 1 for compearing. ...

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• Interball Workshop Posters
• The magnetosphere models
• Space Research Institute (IKI) Seminar

Refinements on precession, Nutation , and Wobble of the Earth VИronique Dehant, Royal Observatory of Belgium ROB rigid Earth nutation Forced Nutations oceanic/atmospheric corrections Non-rigid Earth nutation model Earth response comparison with observation Earth interior model ROB Earth rotation changes due to the core ; core - mantle coupling coupling mechanisms: topographic ...

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• Laboratory of Celestial Mechanics and Stellar Dynamics

. IMA Conference on Multiscale Stochastic Processes Analyzed using multifractals and wavelets, Cambridge UK, March 29-31, 1993. Unpublished. The main results appear in appendix to my `Hamiltonian' paper . Jacques Lewalle, jlewalle@syr.edu

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• Index of /ftproot/users/vab/figure_eos_comparison
• Index of /ftproot/users/vab/figure_eos_comparison/pdf_files
• Index of /ftproot/users/vab/figure_eos_comparison/DOP

paper . Movie 1: BP as seen from EIT, MDI and XRT . Movie 2: BP as seen from TRACE and SOT . Movie 3: MDI and G-band dynamics . Movie 4: Comparison of MDI extrapolated field lines with edge detected images from XRT .

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• J.G. Doyle, Research Astronomer
• Armagh Observatory
• Small-Scale Dynamic Events in the Solar Atmosphere

... 2006 . ... Comparison of total ozone distribution in the high latitudes of both hemispheres SCAR XXIX Open Science Conference, 2006, 12-14 July, Hobart, Australia - Abstract Volume. ... Analyses of spectra, stability and eigenmode transverse small-scale oscillations in the inner Earth magnetosphere. 6th Open Conference of Space Projects Evpatoriya, September 2006, Abstracts . ... Ps6 pulsations in the Earth magnetosphere. 5th Open Conference of Space Projects Evpatoriya, September 2005, Abstracts . ...

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• ION AND ELECTRON ENERGY DETECTOR PAN-2
• Theoretical Astrophysics

... Comparison of simulations with the large scalтАж . Sidebar Left . Sidebar Top . ... Title: Comparison of simulations with the large scale radio galaxy M87. Description: Comparison between a snapshot from Movie 2 (left panel) with the large scale radio structure of the famous radio galaxy M87. ... Comparison of simulations with the large scale radio galaxy M87. Comparison between a snapshot from Movie 2 (left panel) with the large scale radio structure of the famous radio galaxy M87. ...

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• Comparison of a synthetic radio image and quasar 3C 48

... Plasma sheet is the region of closed field lines in the equatorial magnetotail (however, see also plasmoids ). Plasma sheet is typically divided into plasma sheet proper, or central plasma sheet , and plasma sheet boundary layer (PSBL) , the latter being at higher latitudes adjacent to the tail lobes. ... This is evident both in storms time ring current and substorm time plasma sheet (including late growth and the expansion phases; see, e.g., Daglis et al., ... Res., ... J. Geophys. ...

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• Isotropic boundary (Oulu)
• Magnetopause [Oulu]
• Dayside aurora [Oulu]

... Interstellar scintillation of pulsars, interstellar turbulent plasma and supernova Stromgren zones . ... A dependence of the emission measure EM observed in the directions of supernova remnants and pulsars on their ages is derived. The dependence have a well defined low boundary EM min , which increases, when age is decreased. ... The dependence of pulsar pulse broadening tau on pulsar age t have a clearly defined low boundary tau min also. ...

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• UBV light curves (Duerbeck and Walter, 1976)

... 8, PAGES 749-752, AUGUST 1983 A STATISTICAL OF THE STUDY OF THE DYNAMICS OF THE EQUATORWARD BOUNDARY DIFFUSE AURORA IN THE PRE-MIDNIGHT SECTOR J A. Sauvaud J Crasnier 1 Yu I 1, Galperin2, Y I Feldstein 3 1C.E.S.R., CNRS-Universit· Paul Sabatier, 31029 Toulouse, France 2SpaceResearch Institute (IKI), USSR Academy Sciences, Moscow,USSR of 3IZMIRAN,USSR Academy Sciences, Moscow of Region, USSR Abstract. We present a statistical study of the dynamics of the equatorward boundary of the diffuse aurora. ...

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• Empirical Model of the Nighttime Winter Ionospheric Trough
• The 14 July 2000 meter-wavelength dynamic radio spectrum

APPLIED PHYSICS LETTERS 89, 213111 2006 Grain boundary weak link in a-b plane in MgB2 film E. Stepantsov Institute of Crystallography, RAS, Moscow 119333, Russia M. Tarasova Institute of Radio Engineering and Electronics ... Agriculture and Technology, Tokyo 184-8588, Japan D. Winkler Chalmers University of Technology, GЖteborg 41296, Sweden Received 27 July 2006 ; accepted 16 October 2006 ; published online 22 November 2006 The authors have fabricated the ... 89, 213111 2006 FIG. ... FIG. ...

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• INFORMATION SEARCHING SYSTEM "FORGET-ME-NOT" - NDES-99
• Project 7 - INTAS - Dynamics and non-equilibrium transport in advanced
• MAPS WITH STORED INFORMATION IN MULTIPLE-ACCESS COMMUNICATIONS SYSTEMS - NDES...

... 8, ``Celestial Mechanics'', 2002 FCN -- period dependence on dynamic characteristics of a lunar core A. Gusev 1 , N. Petrova 1 , N. Kawano 2 , and RISE group 2 1 Kazan State University, Kazan, Russia 2 National Astronomical Observatory, Mizusawa, Iwate, Japan Two modes in a polar oscillation are obtained when a free rotation of the two--layer Moon was studied: 1 PCW = 2\Omega A Am p fffi ё 1 74yr 1 P FCN = \ Gamma \Omega A 2Am ` C c \ ...

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• http://www.ipa.nw.ru/conference/2002/sovet/PS/KOUPRIAN.PS
• Journe?s 2003
• Journ?es 2003 Second Announcement