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http://www.stsci.edu/documents/dhb/web/c12_fgscalib.fm4.html.

21. Work Scan Program + Data Viewer (IDL widget)
For the calibration of RATAN-600 data you will need to Download Nobeyama Fluxes (1, 2, 3.75, 9.4, 17 GHz): year 1999 2000 2001 2002 2003 . Brief description of Work Scan . Main functions of processing, realized in the program are: . ... Correction of various (not fatal) defects of data; . ... Calculating of the lower enveloping curve or an average scan from observations data for a few days; . ... COMMENT This table contains the set (TFIELDS) of 1-dimensional (TFORM# . ... AZIMUTH = 'float' / . ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/sun/software.htm -- 8.5 Кб -- 24.02.2010
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/sun/software.htm -- 8.5 Кб -- 24.02.2010
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/sun/software.htm -- 8.5 Кб -- 24.02.2010
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22. Olga P. Verkhoglyadova
Large-scale wave processes in space plasma. ... G.V.Lizunov, O.P. Verkhoglyadova, and K.I. Churyumov, Plasma- beam instabilities in comatary ionospheres, Russian Astronomical Journ. ... Verkhoglyadova, O.P., V.V. Grimalsky, Propagation of ion- sound solitons in unhomogeneous plasma, Ukrainian Phys. Journ., ... Verkhoglyadova, O.P., Ivchenko, V.N., Plasma regime identification technique using magnetospheric satellite measurements, Space Sci. and Technology, 4 (5/6), 18-27 (1998) (in Ukrainian). ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/staff/Verkhogl.html -- 14.7 Кб -- 23.01.2004
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23. PolygonFiller (ImageJ API)
... Class . ... PREV CLASS NEXT CLASS . ... CONSTR | METHOD . ... java.lang.Object ij.process.PolygonFiller . public class PolygonFiller . ... This class fills polygons using the scan-line filling algorithm described at "http://www.cs.rit.edu/~icss571/filling/". ... Constructs a PolygonFiller. PolygonFiller (int[] x, int[] y, int n) . ... Constructs a PolygonFiller. public PolygonFiller (int[] x, int[] y, int n) . ... Method Detail public void setPolygon (int[] x, int[] y, int n) . ...
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/process/PolygonFiller.html -- 13.0 Кб -- 02.12.2010
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24. COALA - Computational Astrophysics Laboratory
Chiaki Kobayashi, Ralph Sutherland How galaxies did form and evolution? - to answer this unsolved problem, we are simulating the formation and evolutionary history of galaxies in the Universe, including star formation, supernovae feedback, and chemical enrichment. Comparing the spacial distribution of elements within galaxies with observations, we will examine fundamental physical processes that drive galaxy formation. ... COALA : Universe Galaxy AGN Star Planet ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/coala/galaxy.html -- 5.9 Кб -- 01.10.2012
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25. The dust jets in the nucleus of comet 29P/Schwassmann-Wachmann 1
... An estimate the rotation period of cometary nuclei is important for understanding and describing the physical processes of the cometary activity. Unfortunately, the measurements of the rotation periods of the comet nucleus depend on the model assumptions and it is one of the main reasons for the scatter of the estimates given in various articles for a given comet. ... Right: the image of the comet 29P/Schwassmann-Wachmann 1 obtained at the 6-m telescope. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/SciNews/2012/Ivanova/ -- 5.4 Кб -- 03.02.2013
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/Doc-en/SciNews/2012/Ivanova/ -- 5.4 Кб -- 03.02.2013
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26. http://www.astro.spbu.ru/staff/afk/AtDatCentre/AtDatCat/Introduction.pdf
Introduction This catalogue contains mainly the atomic data needed in the astrophysical investigations of low-density plasma. It is a revised and extended version of the "Catalogue of Atomic Data for the Rarefied Astrophysical Plasma" (Golovatyj et al. ... Low-density plasma. ... In the present study we represent only the atomic data for computation of sp ectra of low-density astrophysical plasma (most known kinds of it are gaseous nebulae), their thermal and ionization structure. ...
[ Текст ]  Ссылки http://www.astro.spbu.ru/staff/afk/AtDatCentre/AtDatCat/Introduction.pdf -- 47.2 Кб -- 19.11.2010
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27. FADPS - Flexible Astronomical Data Processing System
... The reduction system of observations FADPS (description in Russian) (Flexible Astronomical Data Processing System) for data of wide-band receivers of the first observation cabin of the radio telescope RATAN-600 had been created under the Unix-like operational system DEMOS for computers of the SM-1420-type (PDP/11) in 1987 for observation analysis and estimates of coordinates and flux densities of radio sources. ... FADPS: flexible astronomical data processing system at RATAN-600 in UNIX environment....
[ Сохраненная копия ]  Ссылки http://sed.sao.ru/~vo/fadps_e.html -- 15.4 Кб -- 24.02.2010
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28. wave processes
The investigation of features of electromagnetic waves propagation, their generation and absorption in weakly inhomogeneous chiral media were started and the following results were obtained : . the governing equations to describe the electromagnetic waves interaction with inhomogeneous chiral plasmas were derived (together with N.S.Erokhin); . ... it was proven the 100 % hybrid mode conversion in the case of normal waves incidence upon inhomogeneous plasma (together with N.S.Erokhin); . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/mss04/s6.htm -- 2.7 Кб -- 04.03.2004
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/mss04/s6.htm -- 2.7 Кб -- 04.03.2004
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29. Семинар по звездной астрономии
... Архив семинара . ... Triggered Star Formation" . It is now well established that massive stars in star forming regions can trigger next generation of star formation. ... The young stellar objects (YSOs) in star forming regions have been identified using the near-infrared (NIR) and mid-infrared (MIR) observations. ... The age of YSOs, the morphology of the regions and the global distribution of YSOs indicate that the star formation can be triggered by either (RDI/ CC) of the processes. 40 мин. ...
[ Сохраненная копия ]  Ссылки http://lnfm1.sai.msu.ru/~zabolot/proba.htm -- 3.3 Кб -- 29.03.2016
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30. PS_obj.html
... Shematovich, V.I . ... Shematovich, V. I. ; Bisikalo, D. V.; Marov , M. Ya . ... Shematovich, V.I., Bisikalo, D.V., and Gerard J.-C. Superthermal particles in the planetary atmosphere. ... Shematovich, V.I., Bisikalo, D.V., and Gerard, J.-C. The thermospheric odd nitrogen photochemistry : role of non-thermal N(4S) atoms (abstract) . ... Geophys ., ... Gerard, J.C., Shematovich, V.I., and Bisikalo, D.V. Effect of hot N( 4S) atoms on the NO solar cycle variation in the lower thermosphere (abstract) . ...
[ Сохраненная копия ]  Ссылки http://www.inasan.rssi.ru/~shematov/HotAtoms.html -- 71.4 Кб -- 06.04.2010
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31. The /proc filesystem
Next: Using Disks and Other Up: Overview of the Directory Previous: The /var filesystem . The /proc љ filesystem contains a illusionary filesystem. ... Instead, the kernel creates it in memory. It is used to provide information about the system (originally about processes, hence the name). Some of the more important files and directories are explained below. ... Shows which DMA channels are being used at the moment. /proc/filesystems љ . ... An image of the physical memory of the system. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/sag-0.4/node27.html -- 7.3 Кб -- 04.05.1997
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32. Accuracy of World positional CCD observations of the numbered minor planets
... Advises . Contact Advises . As an advise for amateurs we would like to underline: if it's possible, try to observe 3 asteroid positions per night and do not neglect to observe the Numbered Minor Planets in your telescope field of view as a "by product" of your observational programs. ... We think such estimations ought to be produced every morning after CCD observations of the moving celestial objects by observer himself. ...
[ Сохраненная копия ]  Ссылки http://www.accuracy.puldb.ru/ADVISES.HTM -- 2.8 Кб -- 05.12.2007
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33. Optical systems and devices
To main of Laboratory . The research work and design of optical and optical-electronic devices are carries out by laboratory staff: . ... Lens: . ... In the layout 1 prism systems perform functions of dispersive element, corrector of aberrations, optical reducer. ... Spectral range 200 - 400 nm; . ... Back Forward . ... The main corrector's function are compensation of field aberrations of the main spherical mirror of a telescope (diameter of 600 mm, f'=1200 mm) and increase aperture ratio. ...
[ Сохраненная копия ]  Ссылки http://www.mao.kiev.ua/lao/optical_systems_eng.html -- 19.6 Кб -- 12.01.2010
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34. Pulkovo Databases
System of astrometric databases of Pulkovo observatory. 26-inch refractor . Pulkovo system of astrometric databases consists of three databases, which contain results of processing photographic and CCD observations, obtained with the 26-inch refractor and the Normal astrograph of Pulkovo observatory. Pulkovo photographic catalogs: Pul-2, Pul-3 (Pul-3 SE), Pul ERS . Results of photographic and CCD observations of Solar system objects . ... Normal Astrograph ...
[ Сохраненная копия ]  Ссылки http://www.puldb.ru/db/help1.php -- 4.3 Кб -- 01.10.2012
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35. The HST Guide Star Catalog
I/220 The HST Guide Star Catalog (Lasker+ 1992) ================================================================================ The Guide Star Catalog Version 1.1 - An all-sky astrometric and photometric catalog to support the operation of the Hubble Space Telescope The Guide Star Catalog Version 1.0 is described in a series of papers: I. Astronomical foundations and image processing Lasker B.M., Sturch C.R., McLean B.J., Russell J.L., Jenkner H., Shara M.M. =1990AJ.. ... Astrophys. ...
[ Сохраненная копия ]  Ссылки http://vega.inp.nsk.su/catalogs/gsc-description.php3 -- 31.1 Кб -- 01.10.2012
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36. IIS7
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[ Сохраненная копия ]  Ссылки http://platon.asc.rssi.ru/ -- 1.7 Кб -- 26.11.2009
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37. The NMW survey homepage
NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...
[ Сохраненная копия ]  Ссылки http://scan.sai.msu.ru/nmw/ -- 10.7 Кб -- 18.02.2015
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38. XWare > APOD
... Venus, Mercury, and Saturn wandered close together in western evening skies last week. ... Thirteen Million Kilometers from Comet Tempel 1 . ... In the center is a large but peculiar elliptical galaxy dubbed NGC 1316. ... Globular Cluster M22 from CFHT . ... Stars orbit the center of the cluster, and the cluster orbits the center of our Galaxy. ... Venus, the second closest planet to the Sun, is by far the brightest of the three planets gathered in this weekend's western sky at sunset. ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/apod.html?page=7&d=2005-08 -- 15.1 Кб -- 12.04.2016
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39. Obtaining Charts.
... The target area that we are concerned with in this study has a few problems....in that there isn't an abundance of literature available for the individual to access in search of photographs of the target galaxies, and magnitude sequencing of stars around these galaxies. ... The Rev. Robert O. Evans of Coonabarabran, Australia. ... Reference photographs (no sequencing) of the target galaxies (with the exception of 27 galaxies) can be found in the Deep Space CCD Atlas: North, by John C. Vickers.( ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/mirrors/isn/obtcha.htm -- 4.9 Кб -- 02.02.2012
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40. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE6258F57-38C4-495D-9D62-5A27CFF1008B%7D
This illustration shows the disk of our Milky Way Galaxy surrounded by a fain, extended halo of old stars. Astronomers using the Hubble Space Telescope to observe the nearby Andromeda Galaxy serendipitously identified a dozen foreground stars in the Milky Way halo. They measured the first sideways motions (represented by the arrows) for such distant halo stars. The motions indicate the possible presence of a shell in the halo, which may have formed from the accretion of a dwarf galaxy. ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE6258F57-38C4-495D-9D62-5A27CFF1008B%7D -- 4.2 Кб -- 10.04.2016
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