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http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node183.html.
http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node183.html.
21. The summary plot of time distribution of the multisatellites magnetic
The summary plot shows the monthly time distribution of all predicted magnetic conjugations between four spacecraft considered. ... To show the time of conjugation, in frame of the corresponding day for each SC the corresponding colour and line are used: . for the first SC the red color and the first line are used, . ... On the plot the SC names are shown by the corresponding colours. The summary plot permit to find the simultaneous magnetic conjugations of 3 and even 4 satellites. ...
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Ссылки http://www.iki.rssi.ru/vprokhor/descr/sumplot.htm -- 2.5 Кб -- 19.11.1999
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/vprokhor/descr/sumplot.htm -- 2.5 Кб -- 19.11.1999
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[ Сохраненная копия ] Ссылки http://www.cosmos.ru/vprokhor/descr/sumplot.htm -- 2.5 Кб -- 19.11.1999
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22. Explanations for solar physics computing page
This document explains values, tables and other matters on solar physics computing pages. ... is040423.ete : SAHA-S tables, interpolation values: T, rho, X. Z is fixed at 0.02. See reference above. opal2005.etf : OPAL EOS, interpolation values: T, rho, X, Z. Downloaded from OPAL site , marked there as "2005", seems to be unpublished. opal2001.etf : OPAL EOS, interpolation values: T, rho, X, Z. Rogers F.J., Nayfonov A. Astrophys. ... The following values can be calculated: . ... dimensionless . ...
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Ссылки http://crydee.sai.msu.ru/physics/phys-help.html -- 8.0 Кб -- 21.10.2009
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23. (Untitled)
To construct two-dimension distribution of minor planets user should specify elements/ parameters/ function that will be plotted as abscissas and ordinates. In three-dimension case one should add to them the element plotted on Z axis. ... Though you may choose elements plotted along different axes at will, often there is good reason to plot such elements as a, n, or n" along X axis (two-dimension distributions) and to plot them along Y axis in three-dimension case. ...
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Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user8zse.htm -- 3.4 Кб -- 10.04.2016
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24. Relative literature to radio galaxy study
... High redshift radio galaxies . ... Verkhodanov O.V., Kopylov A.I., Zhelenkova O.P., Verkhodanova N.V., Chernenkov V.N., Parijskij Yu.N., Soboleva N.S., Temirova A.V. 2000. ... Verkhodanov O.V., Kopylov A.I., Parijskij Yu.N., Soboleva N.S., Temirova A.V. "Color ages of parent galaxies of high redshift radio sources", in Proc. XV Conf. on "Aktualnye problemy vnegalakticheskoi astronomii" ("Current Problems of Extragalactic Astronomy"), Pushchino, May 25--29, 1998, printed in Pushchino Sci. ...
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25. http://www.mrao.cam.ac.uk/galevol/tgoerdt_Camebridge_2013.pdf
Cold streams: detectability, relation to structure and characteristics Tobias Goerdt Universidad AutСnoma de Madrid with Daniel Ceverino, Andi Burkert, Avishai Dekel, Amiel Sternberg Cold streams Detectability in absorption: Computed sky covering fraction · Very low sky covering fraction · Low metallicity in streams Stacked absorption line profiles · Central geometry / 'down the barrel' · In agreement with Steidel et al. (2010) or BouchИ et al. ...
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Ссылки http://www.mrao.cam.ac.uk/galevol/tgoerdt_Camebridge_2013.pdf -- 1697.8 Кб -- 06.10.2013
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26. Polarization properties (transmitted radiation)
Next: Polarization efficiency: size/shape/orientation effects Up: Optical properties of cosmic Previous: The 2175? feature . To model the interstellar polarization one needs to calculate the forward-transmitted radiation for an ensemble of non-spherical aligned dust grains. ... Let non-polarized stellar radiation passes through a dusty cloud with a homogeneous magnetic field. ... The angle between the line of sight and the magnetic field is ( ). ... where the angle is connected with and ( ). ...
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Ссылки http://www.astro.spbu.ru/DOP/8-GLIB/ASTNOTES/node5.html -- 24.1 Кб -- 19.11.2010
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27. HwB: SGI Mouse (Model 021-0004-002) Connector Connector (Offline)
at the Computer) . 9 PIN D-SUB ??? at the Computer. Pin . ... Not connected . ... Note: Direction is Computer relative Mouse. ...
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Ссылки http://www.arcetri.astro.it/irlab/doc/library/hwbook/connector/userinput/sgimouse0210004002.html -- 3.9 Кб -- 06.07.2001
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28. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE697A649-B990-4F0C-9693-88E72FFCBA78%7D
... The colors indicate the relative motions of galaxies with accurately measured distances, with shades of green and blue indicating motions toward us and shades of yellow to red indicating motions away from us. Our nearest neighbors have only small relative motions (represented by yellows and greens), as seen best in the exploded view of the right panel. We, along with all these nearest neighbors, are moving together toward the lower right corner of the figures. ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE697A649-B990-4F0C-9693-88E72FFCBA78%7D -- 5.6 Кб -- 10.04.2016
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29. Study of radio spectra and variability of GPS sources
... The results of long-term monitoring of Gigahertz-Peaked Spectrum sources were found the statistically significant differences (0.05 significance level) in the high-frequency spectral index distribution between subgroups of galaxies and quasars. ... This can mean that the electron energy distribution for GPS galaxies is steeper than for GPS quasars. ... The first area corresponds to GPS-quasars that have statistically larger value of redfhift, second area corresponds to GPS-galaxies. ...
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Ссылки http://www.sao.ru/Doc-en/SciNews/2011/Mingaliev/ -- 4.9 Кб -- 02.10.2012
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30. MAO NASU :: Topic: The third-order space-by-time relation (1/1)
... Recent Topics . ... MAO main . ... The third-order space-by-time relation . ... Тема: The third-order space-by-time relation . ... The mass m experiences a gravity force toward the sun and . ... will experience the Coriolis force or Coriolis acceleration. ... differentiated space-by-time twice and discovered equation2. ... If one differentiates . ... time differentiation of space-by-time. ... third-order space-by-time relation. ... understand the third-order space-by-time relation. ... MAO NASU . ...
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Ссылки http://www.mao.kiev.ua/index.php/en/forum/info/193-the-third-order-space-by-time-relation -- 23.6 Кб -- 11.04.2016
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31. Ionospheric plasma-wave interaction
. Language [RU/EN] Search: . Home . UP . Research . Projects . Services . Info . News . Events . Personal . Archive . Ionosphere and radiowave propagation: structure . The main page . Information . Publications: . 2011 - 2015 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2000 - 2004 . 1995 - 1999 . Participation in International symposiums and conferences: . 2013 - 2015 . 2011 - 2012 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2002 - 2004 . N.V. Pushkov . 09/04/2016 23:52 MSK . webmaster@izmiran.ru .
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32. Relative pathnames
. You can define a file or directory by its location in relation to your current directory . The pathname is given as / (slash) separated list of the directories on the route to the file (or directory) from your current directory. A .. (dot dot) is used to represent the directory immediately above the current directory. In all shells except the Bourne shell, the ~ (tilde) character can be used as shorthand for the full pathname to your home directory. Examples . Did You Know? .
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Ссылки http://comet.sai.msu.ru/UNIXhelp/concepts/pathfile2.html -- 2.3 Кб -- 17.01.1997
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33. lsst.tcc: python/tcc/mov/pathSegment.py Source File
lsst.tcc љ 1.2.2-3-g89ecb63 . ... Files . FileљList . ... python . tcc . mov . pathSegment.py . ... 22 љ def __init__ (self, pA, vA, pB, vB, dt, doPos): . ... 92 љ # Note that lim (j->0) t_pexArr = - vA / aA, yet the equation used below . ... tcc.mov.pathSegment.PathSegment.pMax . ... Definition: pathSegment.py:83 . tcc.mov.pathSegment.PathSegment.dt . ... tcc.mov.pathSegment.PathSegment.__repr__ . ... Definition: pathSegment.py:130 . ... tcc.mov.pathSegment.PathSegment.aPeak . ...
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Ссылки http://www.apo.nmsu.edu/Telescopes/TCC/html/path_segment_8py_source.html -- 37.2 Кб -- 14.09.2015
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34. http://www.issp.ac.ru/libm/papers/2001-17.pdf
Scripta mater . 44 (2001) 893 897 www.elsevier.com/locate/scriptamat APPLICATION OF THE THERMODYNAMIC THEORY OF IRREVERSIBLE PROCESSES TO NORMAL GRAIN GROWTH P.R. Rios1,2, G. Gottstein1 and L.S. Shvindlerman 1 2 1 Institut fur Metallkunde und Metallphysik, RWTH Aachen, D-52056 Aachen, ... Trabalhadores, 420, Volta Redonda, RJ, 27255-125 Brasil (Received July 26, 2000) (Accepted in revised form November 7, 2000) Keywords: Grain ... Total Grain Boundary Area vs. ... P. R. Rios, Scripta Mater. ...
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Ссылки http://www.issp.ac.ru/libm/papers/2001-17.pdf -- 137.7 Кб -- 25.06.2006
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35. Meade Instruments Corporation - Autostar Computer Controller Instruction Manual
... Meade Instruments Corporation . ... Autostar Computer Controller Instruction Manual . Autostar Computer Controller . ... NOTE: This manual covers both Model #495 Autostar and #497 ETX Autostar Computer Controllers. ... Autostar Primary Menus and Options . ... Chapter 3: Alignment . ... Guided Tour Menu . ... Chapter 5: Autostar Menu Functions . ... Meade Autostar Computer Controller . ... Meade #505 Connector Cable Set Manual . ... Copyright 2006 Meade Instruments Corporation, All Rights Reserved. ...
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Ссылки http://www.meade.com/manuals/autostar/index.html -- 11.8 Кб -- 10.11.2012
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36. atmos 3.0 page
The most up-to-date information related to atmos 3.0 are collected here due to constantly increasing interest to MASS/DIMM processing software... atmos 3.0 is still beta , so the latest version is 2.97.5 (there is also 2.98.x branch which absorbs new features) . ... M' line: . ... free seeing and its relative error . ... dimm seeing and its relative error (if dimm data are present, zeros otherwise) . ... dimm turbulence power and its relative error (if dimm data are present, zeros otherwise) . ...
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Ссылки http://curl.sai.msu.ru/~matwey/atmos/ -- 6.8 Кб -- 05.02.2016
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37. http://www.astro.louisville.edu/software/archive/colorspec/colorspec-1.0/README
Programs to generate color spectra ================================== These programs were developed to produce realistic color spectra from digital data. ... The distribution here contains the original source code for colorspec and solar in C, and a version of solar written in Fortran. ... It will produce a color spectrum of any digital spectrum. ... The 800x50 image solarflux.ppm was generated by colorspec and the file fluxatlas.dat, a reformatted NSO Solar Flux Atlas in the data directory. ...
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Ссылки http://www.astro.louisville.edu/software/archive/colorspec/colorspec-1.0/README -- 4.8 Кб -- 23.08.2004
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38. http://selena.sai.msu.ru/Shev/Publications/ms38/ms083.pdf
Microsymposium 38, MS083, 2003 (A4 format) MERCURY: LOCAL VARIATIONS OF THE PHOTOMETRIC RELIEF. ... Because of trajectory and pointing angle constraints the planet could be observed from Mariner 10 only over a small range of phase angles between about 75o and 110o. Therefore the photometric investigations are restricted to measuring the distribution of brightness on the Mercurian disk. ... Raw versions of real-time processing pictures FDS 0000984 and FDS 0000986 were used (images 196 and 202). ...
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Ссылки http://selena.sai.msu.ru/Shev/Publications/ms38/ms083.pdf -- 346.6 Кб -- 06.10.2008
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39. It Really Is Relative - an Astronomy Net UFO Forum Message
UFO Forum Message . Forums: . ... Post . ... It Really Is Relative . ... Post Message | ... If you are on the Earth the moon does not rotate around its own axis. ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
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Ссылки http://www.astronomy.net/forums/ufo/messages/1050.shtml -- 13.1 Кб -- 09.04.2016
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40. http://www.mccme.ru/~ansobol/otarie/slides/kolesnikov.pdf
Optimal transportation, curvature flows, and related a priori estimates Alexander Kolesnikov Moscow 2010 1 Curvature flow Shrinking family of (convex) surfaces At, where every point x A on the curvature of A at x x = -K (x) · n(x). Here K (x) is the (Gauss) curvature of At at x. Approaches to the curvature flows · 1) Solving a parabolic nonlinear equation with smooth data ( R.S. Hamilton, R. Huisken .. ... curvature flow x = -td where t = (x). ... C1(M ) sup | ... Let F (r, ) be a smooth function. ...
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Ссылки http://www.mccme.ru/~ansobol/otarie/slides/kolesnikov.pdf -- 142.6 Кб -- 21.05.2010
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