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1. Kodak paper comparison tutorial
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. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/drabek/CCDP/TUTORIAL/COMPAR/Tutorial.htm -- 7.2 Кб -- 10.09.1998
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2. Шахов Валентин Гаврилович. Публикации
... 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....
[ Сохраненная копия ]  Ссылки http://www.ssau.ru/staff/61481001-Shakhov-Valentin-Gavrilovich/publ -- 25.0 Кб -- 27.04.2015
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3. STScI Preprint #1198
... 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 . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1198/prep1198.html -- 5.2 Кб -- 23.05.2000
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4. A Statistical Comparison of Line Strength Variations in Coma and Cluster
... 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. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/15_3/jones/paper/index.html -- 52.4 Кб -- 08.04.2016
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5. Interacting Electrons in Normal Metals
... 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. ...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/engl/education/miptsspd/53-interactingelectronsinnormalmetals- -- 17.3 Кб -- 10.04.2016
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6. G74.0-8.5
... 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 . ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs/snrs.G74.0-8.5.html -- 12.2 Кб -- 10.04.2016
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7. Synthetic Images of the Solar Corona from Octree Representation of 3-D Electron
... 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. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass96/llebariaa2.html -- 12.0 Кб -- 23.06.1998
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8. ALFA Pulsar Surveys Jim Cordes, Cornell University GALFA Workshop, Arecibo 20
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 . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/alfa/galfa/meetings/1/talks/psrlong_files/talk.htm -- 2.8 Кб -- 06.05.2003
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9. http://www.puldb.ru/jenam_2011/PUB_JENAM_2011/shakht_2.pdf
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. ...
[ Текст ]  Ссылки http://www.puldb.ru/jenam_2011/PUB_JENAM_2011/shakht_2.pdf -- 328.6 Кб -- 05.01.2013
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10. Events on January 10-11, 1997 - INTERBALL observations
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. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/tail/results/mpcros/index.html -- 8.9 Кб -- 14.02.1997
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/tail/results/mpcros/index.html -- 8.9 Кб -- 14.02.1997
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