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21. Database of Optical Constants -- Level: welcome
The database contains references to the papers, data files and links to the Internet resources related to measurements and calculations of the optical constants in the wavelength interval from X-rays to radio domain. ... References to some useful books and reviews on the subject (e.g. the classical handbooks edited by E.D.Palik) and links to Internet collections of optical constants and personal WWW pages with related software were also placed in the database. You have arrived at our welcome page. ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/JPDOC/ -- 10.8 Кб -- 19.11.2010
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22. MSSA results
initial data . mean 1990-2012 . mean 1970-2012 . PC 1 (1+2) mean . PC 2 (3+4) annual . ... PC 5 (9+10) 1/3 year . ... PC 4 (7+10) quasi-biannual . ... Sum of nine first PCs 2-10 without mean (1st PC) . Difference between the initial signal and ten first PCs 1-10 . ... Sum of ten first PCs 1-10 . ...
[ Сохраненная копия ]  Ссылки http://lnfm1.sai.msu.ru/~tempus/science/MSSA/ATMZ/index.htm -- 5.9 Кб -- 29.11.2012
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23. Spectrum v1 - Examples
In order to calculate the line profile of a given absorption line for atomic species Z with a wavelength LAMBDA (in Angstroms) and a microturbulent velocity VT (in km/s). ... mode . ... 1) The input model may contain more than one model (i.e. it may be an entire grid of models). Spectrum will cycle through this grid NMOD times, omitting NSKIP-1 models from the . ... However, the input data following MODE must be repeated NMOD times in order to obtain equivalent results for each model in the grid. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~csj/software_store/guide/spectrum_v1_examples.html -- 7.6 Кб -- 02.06.2003
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24. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BEF589640-D426-4FC0-B061-129D8CDF2D0C%7D
The maps show how the sky looks at gamma-ray energies above 100 million electron volts (MeV) with a view centered on the north galactic pole. The first frame shows the sky during a three-hour interval prior to GRB 130427A. The second frame shows a three-hour interval starting 2.5 hours before the burst, and ending 30 minutes into the event. The Fermi team chose this interval to demonstrate how bright the burst was relative to the rest of the gamma-ray sky. ... NASA/DOE/Fermi LAT Collaboration ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BEF589640-D426-4FC0-B061-129D8CDF2D0C%7D -- 4.3 Кб -- 10.04.2016
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25. Oct-Nov 2003
. Figure 3. The SOHO/EIT derotated fixed-difference images with 6-hour time intervals in four channels of 304, 171, 195, and 284 illustrating the dimmings in different-temperature lines for two events of the 1st rotation (October 26, 2003 (a-d), November 4, 2003 (e-h)) and one event of the 2nd rotation (November 17, 2003 (i-l)). In frame d, the difference image with a 12-hour interval is presented because the 284 heliogram belonging to October 26, 19 UT is not available. To the parent page .
[ Сохраненная копия ]  Ссылки http://www.izmiran.rssi.ru/~ichertok/0310_11/fig3.html -- 2.2 Кб -- 09.06.2012
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26. http://www.mrao.cam.ac.uk/~rachael/compphys/examples/euler.f90
Program to demonstrate the Euler method on ! dy/dx = y over the interval [0,1] program euler implicit none integer, parameter :: n = 10 ! ... kind for double precision integer :: i ! loop counter real(dp) :: x, y, h ! ... interval spacing h = 1.0_dp / n ! ... open file for results open(10,file='euler.dat') ! ... close file close(10) contains ! this function provides the value of dybydx at (x,y) real(dp) function f(x,y) real(dp), intent(in) :: x, y f = y end function f end program euler ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~rachael/compphys/examples/euler.f90 -- 1.8 Кб -- 18.10.2005
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27. Main
... 30 April 2003 . ... 2003 Paper . SN Ia confidence contours from all sources for Omega Matter and Omega Lambda- Blue contours show 68,95 and 99.7% confidence intervals. ... SN Ia confidence contours from all sources for the equation of state and Omega Matter- Blue contours show the 68, 95 99.7% confidence intervals. ... Coming Soon . ... Best fit model (A), 1-sigma model (B), are shown relative to Concordance Model (C). ... 2003 Paper - w versus Omega_M . ... 2003 Paper - Omega_M versus Omega_L . ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~brian/highz/index.html -- 4.3 Кб -- 01.10.2012
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28. ASP: Guest Observer
... SEARCH ASP SITE: Match ALL words Match ANY word . ... Comet Hyakutake wowed us this spring [see Guest Observer, May/June, p. 11]. ... The best time to observe a meteor shower is after midnight, as your nighttime location moves head-on into the path of the cometary debris. ... As observers, we are interested in the number of Perseids per time interval. ... Tabulate the number of meteors observed per interval, and make sure to label the table with the local time and date of each interval. ...
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/pubs/mercury/9604/perseids.html -- 22.4 Кб -- 20.04.2012
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29. Introduction to dynamical systems (Spring 1999)
... Circle rotations. ... Symbolic dynamical systems: sequence spaces, Markov chains, adding machines. Birkhoff recurrence theorem. ... Tent map. ... Expanding maps of a circle. ... Topological entropy. ... Finiteness of entropy for Lipschitz self-maps. Entropy for symbolical dynamical systems. ... Entropy for one-dimensional maps. Entropy for expanding maps and the Misiurewicz-Przytycki theorem. ... Structural stability of expanding circle maps. ... SRB measures for expanding maps. ...
[ Сохраненная копия ]  Ссылки http://www.mccme.ru/ium/s99/dynsys.html -- 4.5 Кб -- 09.12.2005
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30. Times of minima(maxima) calculator
. Please, enter light elements for your star and Julian Day interval. HJD0: . Period: . JD1: . JD2: .
[ Сохраненная копия ]  Ссылки http://scan.sai.msu.ru/epcalc/ -- 5.8 Кб -- 28.02.2009
[ Сохраненная копия ]  Ссылки http://saistud.sai.msu.ru/epcalc/ -- 5.8 Кб -- 28.02.2009
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31. Mirror baffle measurements
... Secondary Baffle . ... The outside diameter of the tip of ring 5 (the secondary baffle tip) was 1285.7 mm with a range of 0.8 mm p-v. The specifications were 1284.6 and 7.6 mm respectively. ... The outside diameter of the base of ring 5 was 1273.4 mm with a range of 2.0 mm p-v. The specifications were 1272.1 and 8.1 mm respectively. ... The inside diameter of the tip of ring 19 (the primary baffle tip) was 857.7 mm with a range of 0.8 mm p-v. The specifications were 858.0 and 8.6 mm respectively. ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/SDSS/eng.papers/19970703_MirrorBaffles/19970703.html -- 10.2 Кб -- 19.05.1998
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32. Guidelines for creating a password
. choose a word from a dictionary . use personal information such as your name, make of car etc. tell anyone your password . write your password down anywhere . use the password you were given when you first got your account on the system . choose an obscure password preferably between 6 and 8 characters in length, of mixed case and containing at least one non-alphanumeric character such as ! or @ . change your password at regular intervals .
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/UNIXhelp/basics/basic3.2.html -- 2.1 Кб -- 17.01.1997
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