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21. http://www.naic.edu/~phil/lbw/resonance/lbwresonances.html
... plots of rms/mean by channel . bandpasses for the individual 25 Mhz bands where the resonances occur . ... A simplified model of the system temperature including these resonances is: Tsys= Tomt*alpha + (1-alpha)*Tsky + Tamp. ... If you are on cold sky then Tsky may be 6+ 14(scattered)=20 K while the OMT temperature is about 100 K. If you look at a 12 jansky source then Tsky= 20+12*10= 140K is greater than Tomt so Tsys will have a negative going bump at the resonance frequency. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/lbw/resonance/lbwresonances.html -- 6.1 Кб -- 08.04.2002
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22. Format of data description
... Here is an example of the output header of CATS data. ... SIMPLE=T / BITPIX=8 / character information NAXIS=0 / no image data array present EXTEND=T / may be standard extensions OBJECT= CATS SEARCH / CATS search result ORIGIN=SAO RAS DATE=01/01/1997 / date of file creation END XTENSION=TABLE / F-file table extension BITPIX=8 / 8-bits ... NAXIS1=93 / No. of characters per row NAXIS2=1000 / the number of lines (sources) TFIELDS=10 / there are 16 fields per row EXTNAME= CATS / object name: ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/vch/Publications/Eng/html/adbis97/node3.html -- 6.4 Кб -- 28.12.2007
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/vch/Publications/Eng/html/adbis97/node3.html -- 6.4 Кб -- 11.09.2010
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/vch/Publications/Eng/html/adbis97/node3.html -- 6.4 Кб -- 02.10.2012
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23. Database of Optical Properties
Next: Examples of data contained Up: Electronic database Previous: Future plans . In astrophysics, the optical constants mainly are used to calculate the optical properties of scatterers, i.e. cross-sections, scattering matrix, etc. ... Optical properties derived from such models have been discussed in some books (see, e.g., [ 2 , 3 ]) and in principle can be calculated by using various light-scattering tools which are freely available via the internet [ 4 ]. ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/DOP/5-OPTC/JPDOC2/node5.html -- 6.0 Кб -- 19.11.2010
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24. Mikhail V. Goryachev
. Investigation of the physical and chemical properties of the soil planets, moons and asteroids remote methods. I have worked on the development of spectropolarimeters, CCD instrumentation, microcontrollers, etc. Photograph album . Gallery . Address of E-mail . Return . Department of Lunar . and Planetary Research .
[ Сохраненная копия ]  Ссылки http://selena.sai.msu.ru/Gor/GorE.htm -- 5.4 Кб -- 14.05.2014
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25. The Astronomy Shop - Books - by Astronomy Net
The Astronomy Shop . ... AstroGuide | ... Books | NightWatch - A Guide to Skywatching and Astronomical Equipment . ... NightWatch has earned its reputationas a simplified yet complete resource. ... Includes simplified starcharts, updated planet and eclipse information good through the year 2010.10x 10.5. 176 pgs. ... www.astronomy.net . ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.net/shop/books/index.html?item=39 -- 12.0 Кб -- 09.04.2016
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26. http://star.arm.ac.uk/~ambn/abstract286.html
We present simultaneous ultraviolet and optical observations of five flares on the very late type M dwarf Gl 866 (dM5.5e). A procedure to estimate the physical parameters of the flaring plasma has been developed using a simplified model of the flare and a comparison of observed and computed Balmer decrements. With this procedure we have determined the optical thickness, electron temperature and electron density of the flaring plasma at flare maximum for three spectroscopically observed flares. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~ambn/abstract286.html -- 1.6 Кб -- 06.05.1998
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27. http://crydee.sai.msu.ru/ftproot/pub/comp/os/os2/hobbes/incoming/Lzd-v0.5-os2.txt
... Studying its source is a good first step to understand how lzip works. ... Lzd will correctly decompress the concatenation of two or more compressed files. ... Proposed directory for placement: /pub/os2/dev/util Your name: Elbert Pol Email address: elbertdotpol@gmail.com Program contact name: (same) Program contact email: (same) Program URL: (none) Would you like the contact email address included in listings? yes Operating System/Version: Additional requirements: Replaces: (v1.14) ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/ftproot/pub/comp/os/os2/hobbes/incoming/Lzd-v0.5-os2.txt -- 2.7 Кб -- 02.10.2013
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28. http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.1/xmccd-4.1e/libsbig/LinuxDevKit/release/udev/52-sbig-suse-debian.rules_blocked
... If not there, the ST-402 family cams. will not work # properly. ... Pre-renumeration device IDs: #================================ # SBIG ST-7/8/9/10/2K cameras ACTION== add , SUBSYSTEM== usb_device , ATTRS { idVendor }== 0d97 , ATTRS { idProduct }== 0001 , \ RUN += /sbin/fxload -I / lib / firmware /sbigucam.hex -D $env{DEVNAME} # SBIG ST-L cameras ACTION== add , SUBSYSTEM== usb_device , ATTRS { idVendor }== ...
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.1/xmccd-4.1e/libsbig/LinuxDevKit/release/udev/52-sbig-suse-debian.rules_blocked -- 3.8 Кб -- 27.09.2011
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29. http://www.mccme.ru/albio/slides/panteleev.pdf
... The problems of complexity in coagulation: specification 1. ... Numerical experiments Task 1: Activation threshold Final clot density VS activation : model reduction Factor V is activated 7 6 7 6 No factor V activation Fibrin 4 3 2 1 0 0.00 0.02 0.04 0.06 0.08 0.10 0.12 Fibrin 5 5 4 3 2 1 0 0.00 0.02 0.04 0.06 0.08 0.10 0.12 Activation Activation y= Ae ( Bx 1 ) y = Ax Final clot density VS activation : the experiment Fibrin clot density (a.u.) 1.0 0.8 0.6 0.4 0.2 ...
[ Текст ]  Ссылки http://www.mccme.ru/albio/slides/panteleev.pdf -- 2897.4 Кб -- 09.10.2008
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30. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD94528DE-0911-4BCD-A016-5A72BE25B573%7D
. This animation shows a simplified model of the varying temperature data at yearly intervals. The latitude banding has been smoothed to more clearly show the how Titan's peak temperature moves from 19 degrees south to 16 degrees north latitude between 2004 and 2016. The small globe in the upper right corner shows the view of Titan as seen from the direction of the sun. The latitude on Titan where the sun is directly overhead (the subsolar latitude) is indicated by a yellow star. NASA/JPL-Caltech/GSFC
[