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21. Hilbert's 16-th and Related Problems in Dynamics
. This page uses frames. Please browse this page with frame supporting browsers.
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Ссылки http://www.mccme.ru/hilbert16/ -- 1.5 Кб -- 22.12.2002
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22. Phil Plait's Bad Astronomy: Mad Science
... Bad Astronomy . ... Mad Science . ... How fast must an object be travelling so the sound I perceive as it directly passes me will drop in pitch exactly one octave? ... When an object is moving past another object, any sound emitted by the first object is changed in pitch due to the relative motion. ... wl(emitted)" is the wavelength of sound emitted by the object at rest, "wl(heard)" is the wavelength you hear from the object, "v" is the velocity of the object, and "c" is the speed of sound. ...
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Ссылки http://www.badastronomy.com/mad/1997/doppler.html -- 21.9 Кб -- 09.04.2016
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23. Meade Instruments Corporation - Pictor Manual Part 3
... Meade Instruments Corporation . ... Section 3: File Menu . ... Displays the dialog to open an existing image: . ... Saves the current image as a new file name or new file type, or both. ... This can be useful to prevent having 20 or more images open at once, and saves having to close them manually. ... This is done by creating a text file with the same name as the image file. ... Note that Image Information is saved within the FITS file, so there will not be a text file to accompany these files. ...
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Ссылки http://www.meade.com/manuals/pictor/pictor3.html -- 13.0 Кб -- 01.02.2006
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24. More Compiliation Problems - an Astronomy Net XEphem Forum Message
XEphem Forum Message . ... More Compiliation Problems . ... when I compile the Xephem source code in the /GUI/xephem file, I get the following... gcc -O2 -fno-strength-reduce -I../../libastro -I/usr/X11R6/include -I/include -Dlinux -D__i386__ -D_POSIX_C_SOURCE=199309L -D_POSIX_SOURCE -D_XOPEN_SOURCE=500L -D_BSD_SOURCE -D_SVID_SOURCE -D_REENTRANT -DFUNCPROTO=15 -DNARROWPROTO -c aavso.c -o aavso.o . aavso.c:20: Xm/Xm.h: No such file or directory . ... www.astronomy.net . About Astronomy Net | ...
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Ссылки http://www.astronomy.net/forums/xephem/messages/81.shtml -- 14.9 Кб -- 09.04.2016
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25. Astrophysical Research Consortium - Apache Point Observatory
... How do have my images go into a different directory? To put your images into a directory other than the standard /export/images you MUST create the directory from the dryrot prompt. ... Create the directory with the following command dryrot: mkdir /export/images/ your directory Now when you set up the directory in spicam you need to type spicam: path /export/images/ your directory This will now put the images into your directory. ...
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Ссылки http://www.apo.nmsu.edu/35m_operations/35m_manual/Instruments/SPIcam/SPIcam_problems.html -- 4.9 Кб -- 07.03.2007
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26. University Problem Based Learning Exercises for Teaching Astronomy and Physics
... The Australian National University] [Department of Physics] [Paul Francis] [Main Roleplay Page] . These exercises are my attempt to adapt the technique of Problem Based Learning to the context of introductory astronomy and astrophysics classes. ... As students grapple with the puzzle, they are forced to learn the subject matter of the course. ... This exercise is designed for 1st year University students with a reasonable high-school background in Maths and Physics. ...
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Ссылки http://www.mso.anu.edu.au/pfrancis/PBL_copies.html -- 8.0 Кб -- 01.10.2012
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27. A New Stable Method for Long-Time Integration in an N-Body Problem
Next: Imaging by an Optimizing Method . ... A big advantage of this numerical integrator is its stability: the error in the semi-major axis and the eccentricity depends only on the step size and does not grow with an increasing number of time steps. ... As the integration time increases, the numerical results become more contaminated by various errors. ... A new symplectic integrator produces no secular truncation errors in the actions of a Hamiltonian system. ...
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Ссылки http://www.adass.org/adass/proceedings/adass96/taidakovat.html -- 9.4 Кб -- 23.06.1998
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28. CURRENT ASPECTS OF REMOTE SENSING OF EARTH FROM SPACE
... CURRENT ASPECTS OF REMOTE SENSING OF EARTH FROM SPACE . ... For developing of the scientific concept and the programs of global monitoring of the Earth from space and pursuant to the disposal of Presidium of Russian Academy of Sciences # 10310-717 (August 11, 2004 ) Space Research Institute RAS and Center of Space Observations of the Russian Space Agency during November 16-18, 2004 conduct the Second Opened All-Russia conference ' Current Aspects of Remote ...
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Ссылки http://www.iki.rssi.ru/d33_2004e.htm -- 8.6 Кб -- 11.11.2004
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/d33_2004e.htm -- 8.6 Кб -- 11.11.2004
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[ Сохраненная копия ] Ссылки http://www.cosmos.ru/d33_2004e.htm -- 8.6 Кб -- 11.11.2004
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29. http://hea.iki.rssi.ru/conf/hea2007/bbclone/doc/install.txt
... index.php (1) | bbclone/ | ... To do you can use the following sample and point your browser to it. <?php define("_BBC_PAGE_NAME", "Test"); define("_BBCLONE_DIR", "bbclone/"); define("COUNTER", _BBCLONE_DIR."mark_page.php"); if (is_readable(COUNTER)) include_once(COUNTER); ?> ... Create the file "count.php" and add the following: <?php define("_BBCLONE_DIR", "/the/path/that/leads/to/bbclone/"); define("COUNTER", _BBCLONE_DIR."mark_page.php"); if (is_readable(COUNTER)) include_once(COUNTER); ?> ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2007/bbclone/doc/install.txt -- 9.1 Кб -- 13.03.2005
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30. IV International Astronomy Olympiad, Problems to solve
IV International Astronomy Olympiad . ... Text of these problems is available also . ... To solve every problem you may use constants and well-known values you know by heart. ... The apparent diameter of the Moon, as seen from the Earth, is 31'. ... Can you observe a star with magnitude . ... Consider the stars as black bodies. ... Estimate the diameter of a black hole constructed using this patent from a ship with the mass of 5000 tn (1 tn = 1000 kg). ... What stars would you observe this nigth? ...
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Ссылки http://www.issp.ac.ru/iao/1999/problems/vi99us_e.html -- 11.5 Кб -- 15.04.2011
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31. http://www.astro.louisville.edu/software/sbig/xmccd-5.1/REMOTE
Using XPA remotely ================== XPA starts by default using network communication with access control. ... Copy and append id_dsa.pub to $HOME/.ssh/authorized_keys on the system you are connecting to. ... If you are connecting from an observer's computer to a telescope computer that is not on a local area network, you may also need to change the firewall settings to enable SSH. ... The ssh command forward the port 5901 on your local computer to the same port on the telescope computer. ...
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Ссылки http://www.astro.louisville.edu/software/sbig/xmccd-5.1/REMOTE -- 9.0 Кб -- 18.06.2015
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32. VaST homepage
... VaST is a software tool for finding variable objects on a series of astronomical images. ... VaST performs object detection and aperture photometry using SExtractor on each image, cross-matches lists of detected stars, performs magnitude calibration with respect to the first (reference) image and constructs a lightcurve for each object. ... VaST FITS image viewer ./pgfv . ... Part I" PZP, vol. ... K. V. Sokolovsky, S. A. Korotkiy; "New Variable Stars Discovered by the NMW Survey" PZP, vol. ...
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Ссылки http://scan.sai.msu.ru/vast/ -- 122.2 Кб -- 21.02.2016
[ Сохраненная копия ] Ссылки http://saistud.sai.msu.ru/poisk/ -- 122.2 Кб -- 21.02.2016
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[ Сохраненная копия ] Ссылки http://saistud.sai.msu.ru/poisk/ -- 122.2 Кб -- 21.02.2016
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33. http://zebu.uoregon.edu/~uochep/talks/talks02/G020051.pdf
LIGO-G020051-00-Z Isabel Leonor (w/ Robert Schofield) University of Oregon LIGO Reduced Data Sets E7 standard reduced data set RDS generation for future runs decimation examples Standard RDS Guidance from LSC White Paper Data set levels outlined in LSC white paper: Level 0: Full IFO data stream (not archived) Level 1: Archived reduced data set · all important IFO and PEM channels · used principally for detector diagnostics Level 2: IFO strain and ...
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Ссылки http://zebu.uoregon.edu/~uochep/talks/talks02/G020051.pdf -- 1478.3 Кб -- 25.09.2002
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34. New Mirrors
... Make a new empty directory; you'll need about 6 megabytes; . ... Customize "host.html" as described below (optional); . ... Send some mail to me ( billa@znet.com ) with the URL of your new copy so I can update the mirror list; also let me know if you would like to receive email notifications of future updates. ... Several of the mirror sites are using the "mirror" package to keep their copies of TNP up to date automatically instead of waiting for me to send these notices. ... Mirrors .. ...
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Ссылки http://www.iki.rssi.ru/nineplanets/newmirrors.html -- 7.1 Кб -- 30.01.1997
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35. http://www.gao.spb.ru/russian/psas/ffk2013/tfiles/Karshenboim_ffk2013.pdf
... The lines ( ) are equations: e.g., theoretical expressions for h/M, the Lamb shift, .. Some data are measured, a lot are derived: mp [kg], me [Mev/c2], .. ... for a `theoryґ for QHE steps rational universal relation to Needs for a `theoryґ for QHE steps rational universal relation to h block known from block input : h e NA h·NA h/me output me µB h block h block h block : the most important da t a h block : the most important da t a watt ballance Avogadro ...
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Ссылки http://www.gao.spb.ru/russian/psas/ffk2013/tfiles/Karshenboim_ffk2013.pdf -- 1352.2 Кб -- 25.11.2013
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36. State of the problem
Next: Initial conditions Up: Old neutron star distribution Previous: Introduction . The problem to be solved is to find stationary space distribution of stars which have had certain initial space and velocity distributions and move in a given potential. ... In principle, the most straightforward way to obtain the solution is to integrate directly the equations of motion for a sufficiently large number of stars with different initial conditions. ... Then space density is given by . ...
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Ссылки http://xray.sai.msu.ru/~mystery/articles/old_ns/node3.html -- 9.4 Кб -- 19.08.1996
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37. SPUTNIK home page
.
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Ссылки http://sputnik.infospace.ru/goms/engl/goms.htm -- 7.3 Кб -- 14.01.2004
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38. Rayleigh and Rayleigh-Gans-Stevenson approximations
... The possibility to use the electrostatic approximation to calculate the polarizability allows one to consider practically any shape scatterers - from the regular ones (ellipsoid, cylinder, disc) [ 7 , 274 ] to those with an arbitrary shape, structure and anisotropy [ 308 , 309 , 313 , 405 ] (in the last case the polarizability tensor should be found numerically) - using the theory of the Rayleigh scattering. ...
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Ссылки http://www.astro.spbu.ru/DOP/3-REVS/KHLEB1/node12.html -- 7.7 Кб -- 19.11.2010
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39. IDL programs
... This program was created for correlating chosen regions in the series of fts images. ... Chosen regions' . ... In this section the program counts the integral for each region of the grid for each image. ... As a matter of fact, the integral is total brightness of the region and it is counted by 'int_tabulated' IDL function. ... In addition, the program will show the count of the regions which correlate with the corresponding region (the brighter region means the bigger count) and its contour. ...
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Ссылки http://lnfm1.sai.msu.ru/~kupry/SOFTWARE/korel_en.html -- 9.9 Кб -- 15.08.2003
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40. ALIGNASN (Nov98) --- nictools --- ALIGNASN (Nov98)
alignasn -- Change the relative shifts in association file alignasn association . ... calnicb style association file with list of images to be aligned. ... Interactive program to compute relative shifts of images in an association file. ... After computing the relative shifts of the direct images, alignasn searches for corresponding grism images for each of the direct images. ... The grism association is then updated with the same relative shift measurements as determined from the direct images. ...
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Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/nictools/alignasn.hlp.html -- 2.5 Кб -- 06.06.2006
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