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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. ...
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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 . ...
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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. ...
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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 ...
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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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- http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BAD0C7354-4B3B-4B54-8AA4-00BC13828518%7D
- http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD94528DE-0911-4BCD-A016-5A72BE25B573%7D
- http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B63D833D8-103D-4FA8-87FF-FEFAD684280D%7D
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 .
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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 ...
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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 . ...
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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. ...
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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. ...
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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: .
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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. ...
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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 .
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Ссылки http://comet.sai.msu.ru/UNIXhelp/basics/basic3.2.html -- 2.1 Кб -- 17.01.1997
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33. Vertical Structure, figures
... The observed distributions of stars of different ages and metallisities in the Z coordinate relative to Sun: (a) young ( t 3 Gyr) metall-rich ( [Fe/H] -0.13 ) stars; (b) young metal-poor ( [Fe/H]<-0.13 ) stars; (c) old ( 3 Gyr) metal-rich stars, and (d) old metal-poor stars. ... next figure | previous figure . ...
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Ссылки http://ip.rsu.ru/~marsakov/paper2/p2fg2_1.htm -- 2.5 Кб -- 02.02.2007
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34. East Siberian Center for the Earth's Ionosphere Research. Maximum usable
Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... The on-line prediction procedure is based on the Newton interpolation formulae for a uniform distribution of the variable with first, second and third argument powers restrictions (Kurkin V.I. , Polekh N.M., Tchistyakova L.V. MAF operative prognosis for oblique ionosphere sounding// Issledovaniya po geomagnrtismu, aeronomii i phisike Solntsa. ... Prediction MUF calculation for the next 15 minutes; . ...
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Ссылки http://rp.iszf.irk.ru/esceir/lchmen/op_proghen.htm -- 4.8 Кб -- 02.06.2001
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35. Reduction quantities for Dynamical time. Explanations for Computer Ephemeris.
Computer Ephemeris. Reduction quantities for Dynamical time. Explanations. Each row contains for the date specified at 0 h of Time Dynamical Terrestrial: . interval from date to mean epoch T m expressed in julian years, . reduction quantities A+A', B+B', C, D, (all in seconds of arc), E (in 0.0001s), A' , B' (in 0.001). The same table, but for moments, expressed in Sidereal Dynamical Time is to be found on 'Reduction. Sidereal time.' page. ...
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Ссылки http://space.univ.kiev.ua/ephem/exp/Ea3.html -- 2.2 Кб -- 16.10.2004
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36. Rocket Trails in the Milky Way
... Rocket Trails in the Milky Way . ... 29.03.2012 . ... Credit Copyright: Jerry Lodriguss ( Catching the Light ) Explanation: On March 27, five sounding rockets leapt into early morning skies from NASA's Wallops Flight Facility in Virginia. ... Releasing a chemical tracer they created luminous white clouds within Earth's ionosphere at altitudes above 60 to 65 miles, swept along by the poorly understood high-altitude jet stream . ... March . ... March 2012 . ... 2011 2012 . ... NASA Official: Jay...
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Ссылки http://www.astronet.ru/db/xware/msg/apod/2012-03-29 -- 14.2 Кб -- 29.03.2012
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37. RTT150 telescope: GRB 060526
... Observations of GRB afterglows with Russian-Turkish 1.5-m Telescope (RTT150) . ... The afterglow light curve was measured in detail starting from about 5 h after the GRB and over five ensuing nights. In addition, upper limits were obtained on the rapid variability of the afterglow on the first night of observations and the history of afterglow color variations was measured in detail. ... 2007) : . ... Astronomy Letters, 33, 797 (2007) , arXiv:0802.1635 , The original text in Rissian . ...
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Ссылки http://hea.iki.rssi.ru/grb/060526/indexeng.html -- 4.7 Кб -- 17.12.2015
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38. Metagalaxy sector, archive 1996
... Telescopes . ... 1996: . A giant cloud of neutral hydrogen was detected resulting from the observations with the 6-m telescope and other world telescopes in a broad wavelength interval from UV to radio. ... Statistically significant deviations from the Poisson distribution are found in the radiosource distribution within the deep surveys conducted at RATAN-600 at the scales coinciding with those of the recently detected Sakharov oscillations (0.7-0.3 o ). ... Archive . ...
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Ссылки http://www.sao.ru/Doc-en/Science/results/ar_metagal/res1996.html -- 5.7 Кб -- 10.04.2016
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39. Document Title
... The acquisition data base of meteorological temporal data including systematic and chronologic cataloque for Global Tropical Cyclogenesis (on the whole of World Ocean's aquatorium) for 1983-1992 time interval is developed and based on personal computer IBM PC/AT. ... The data base consists of the following units: 1. ... This data base offers a unique opportunity to analyze macro- and synoptic-scale temporal features of global tropical cyclogenesis as indivisible physical process. ...
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Ссылки http://smis.iki.rssi.ru/partners/esharkov/ -- 5.0 Кб -- 06.08.2001
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40. http://www.astro.louisville.edu/shared_skies/archive/select/asteroids/iris/20110406/notes.txt
Date: Night of local time 2011-04-06 to 07 Telescope: CDK125 Camera: Nikon D200 Observer: John Kielkopf Sequential exposures of 7 Iris See 7_iris_15s_12800iso_20110406.gif for a movie of the movement of the asteroid over the time interval lasting about one hour: Thu, 07 Apr 2011 03:22:51 GMT Thu, 07 Apr 2011 04:29:15 GMT
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Ссылки http://www.astro.louisville.edu/shared_skies/archive/select/asteroids/iris/20110406/notes.txt -- 1.3 Кб -- 07.12.2015
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Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
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