Revolution: 1900 . POS_1900_240410_183_00_0002.XMM . ... 2010-04-24 | ... PSF version: 1900_04.PSF . ... Slew: 4012 secs . ... Obs_dur: 94400 secs . ... 004: 93386 sec . ... 005: 93381 sec . ... Full Frame . 001: 93247 sec . ... 002: 93252 sec . ... Full Low . 006: 3868 sec . ... 09:52:34 ... exp continues . ... Ext Full Fra . 003: 89607 sec . ... 007: 6959 sec . ... 008: 6959 sec . ... 009: 8759 sec . ... 010: 6959 sec . ... 011: 6965 sec . ... 012: 6959 sec . ... 013: 6959 sec . ...

... Classes . Files . ... Class List . ... casa . casa::Exp< T, RES > . ... More... #include < Functors.h > . ... Definition at line 378 of file Functors.h . template<typename T , typename RES = T> . RES casa::Exp < T, RES >::operator() . ... Definition at line 380 of file Functors.h . References casa::exp() . The documentation for this struct was generated from the following file: . casa/BasicMath/ Functors.h . ... Generated on Fri Sep 3 2010 13:08:00 for casacore by 1.7.1 ...

Les aurores sont vues seulement dans les r gions polaires ou pr s des p les. ... Il restait une nigme. Les explorateurs polaires avaient rapport que les aurores taient extr mement rares pr s des p les magn tiques eux-m me. ... D'un autre c t , les lectrons de la pluie polaire qui venaient apparemment du Soleil, furent en effet trouv s dans des taches entourant les p les magn tiques, exactement comme les taches de lumi re que Birkeland observa sur sa terrella. ...

... 2.1). ... 2.1.1) : (1.3) a U 3 exp - . ... max . max = const . ... 2 V c3 (2.8), , (2.3) dpxdpydpz = p2 dp sin d d : d dpx dp y dpz dx dy dz = h3 h3 dN d. , , V dpx dpy dpz V dpx dpy dpz /h3. dN = 0 sin d d = 4. 0 2 , p dp 4p2 dp. p=/c : p dp = 2 d, c 2 3 V d : dN = V 2 d . ... kT >> kT С n T >> 1 < E >= T << n exp ( - T ) << 1 < E >= exp ( - T ) << U d = 3 exp(­/T) d/( 2c3) U d = 2 T d/(2c3) . ... 3) U W T =2 c 3 3 2 f W ( x ), f W ( x) = x 3 e - x f W( x) W (7.5) xmax = 3 . ...

cal_exp_sum_rpt (version 12/03/07) . ... Generate a report summarizing the exposures on a calendar by . ... Don Chance . ... 12/03/07 Chance Initial implementaion. Modules . ... report (calendar, output) . Write the report to fileId . run (*args) . Produce a summary report for the exposures on a calendar . ... do cal_exp_sum_rpt [-outfile=<file>] <calendar_name> . ... outfile defaults to the screen . ... version__ = '12/03/07' ...

... Select formula of fitting with: lin+exp-x lin+exp+x lin parabolic 0 1 2 3 . 0)All weights=1; (1) weights=1/rel_err; . ... 0011+47 0559-05 1508+55 1737-30 1820-14 1846-06 1916+14 2022+50 0031-07 0609+37 1530+27 1738-08 1820-30B 1848 +04 1917+00 2027+37 0037+56 0611+22 1540-06 1740-03 1820-31 1848 +12 1918+19 2035+36 0045+33 0621-04 1541+09 1740-13 1821+05 1848 +13 1918+26 2036+53 0052+51 0626+24 1552-23 1740-31 1821-11 1849+00 1919+14 2043-04 0053+47 0628-28 1552-31 1742-30 1821-19 1851 ...

... Ho G N , H o ~ 10 - 42 GeV , . ... M 2 1 = 64G - + 2 2 F 2 ( p'k )( p k ')+ ( 2 1 p 'k ')( p k ) - - + m 2 (k k ') , 2 (11) 19 , , ( « m) 2 2 4GF 2 1 21 = - + + - - + . ... Koryukin V.M. The confinement and the dark matter of the Universe // In the book: Relativistic Nuclear Physics and Quantum Chromodynamics: Proceedings of the XIX International Baldin Seminar on High Energy Physics Problems (Dubna, September 29 ­ October 4, 2008). Dubna: JINR, 2008. ... V.M. Koryukin, Russian Physics Journal. ...

... All images on this page are copyright Robert H. McNaught. ... There have been so many requests for high resolution copies of these images that I ask that all enquiries for these to go directly to Science Photo Library. C/2006 P1 on Jan 18, 10:22 UT. Photo: R. H. McNaught, Siding Spring Observatory. Canon 5D, 135mm, f/2.0, 2 sec exp., ISO 1600 . ... ISO 200 . ... Canon 5D, 50mm, f/2.0, 30 sec exp., ... Canon 5D, 135mm, f/2.0, 120 sec exp., ... Canon 5D, 50mm, f/2.0, 110 sec exp., ...

... Product of two Gaussians · g = N(µ,2) N(µ,2) exp [-(x-µ)І/2І - (x-µ)І/2І] · µ = (µІ+µІ) / (І+І) ; І = ІІ / (І+І) for , µ µ and · g = (1/2) exp [-(x-µ)І/2І] (1/2(І+І)) exp [(µ-µ)І/2(І+І)] Bayesian Aperture Photometry (Gaussian) · Measurements: Background in an area AB = rAS: fB ± B M ( Source + Background ) in an area AS: fM ± · Priors: p(b) = N(b;f0B,0BІ) p(s) = N(s;f0S,0SІ) · Likelihoods: f(fB,B|b,r) exp [-(rb-fB)І/2BІ] ...

Скупка hp картриджей продажа и заправка картриджей. Руководители и К. Морской бинокуляр, фотоаппарат "Зенит 12XP", пленка Fuji 200 . UT 18:13:16, exp 1/125 c . UT 18:48:10, exp 1/30 c . ... Телескоп "Алькор", фотоаппарат "Зенит", пленка Kodak 200 . ...

... public class CurveFitter . ... static int . ... Field Detail public static final int STRAIGHT_LINE . ... public static final int POLY2 . ... public static final int POLY3 . ... public static final int POLY4 . ... public static final int EXPONENTIAL . ... public static final int POWER . ... public static final int LOG . ... public static final int RODBARD . ... public static final int GAMMA_VARIATE . ... public static final int LOG2 . ... public static double f (int fit, double[] p, double x) . ...

... 1621, 2015 April 20 Conrmation of Pulsed Radio Emission from the Pulsar J1907+0919 (Shitov Radio Pulsar, SGR 1900+14) A.P. Glushak, B.Ya. ... Observations at a frequency of 111 MHz with the Large Phased Array at the Pushchino Radio Astronomy Observatory of the Astro Space Center of the P.N. Leb edev Physical Institute conrm the pulsed radio emission of the X-ray pulsar J1907+0919 that is a counterpart of the magnetar SGR 1900+14. ... The average p erio dogram of PSR J1907+0919 is shown in Fig. ...

... Размер BRAND: 33 (21,5 см) . ... Цвет: розовый . ... Джинсы . ... Размер RU: 46 . ... Артикул: X12891 Цвет: красный Состав: 80% полиэстер, 20% эластан; вставка - 100% полиэстер Параметры изделия: для размера 44/50: обхват груди 96-100 см, длина изделия по спинке 28 см Уход за изделием: стирка при 30њС Страна дизайна: Германия Страна производства: Тайланд Упаковка: пакет . ... Размер INT: 50 . ... Queen News Of The World (2011 Remastered) CD . ... Штанишки на широком поясе для девочки Моя любовь. ...

... Геодезические. ... Задача 1. ... M как exp p () =  (1); где  2 T p M; а  (t) геодезическая выходящая из p с вектором скорости : На лекции мы доказали, что экспоненциальное отображение является диффеоморфизмом достаточтно малой окрестности U нулевого вектора из T p M на свой образ exp p (U ): Тогда экспоненциальное отображение вводит так называемые геодезические координаты в окрестности p следующим образом. ...

... For example, the previous examples are periodic. Example Dual beam calibration observation of a strong-point source with the GBT: Example Dual beam calibration observation of a strong-point source with the GBT: 0 -1 -2 Tb -3 -4 0 1000 2000 3000 t 4000 5000 6000 Example 1/f spectrum Shor t section of the data away from the strong source Time stream Power spectral density -1.75 -1.76 -1.77 -1.78 -1.79 240 260 280 300 t 320 340 360 15 5 5 15 25 0.0 0.2 0.4 Frequency 0.6 Power ...

exp. energy levels: Martin,W.C., Sugar,J., Musgrove,A., Dalton, G.R., 2000, NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61. %exp. energy levels (1s2p 3P): Curdt, W., Landi, E., Wilhelm, K., Feldman, U., 2000, Phys.Rev.A, in press %Comment: the 1s2p 3P energies are calculated using the 1s2s 3S level as reference. ... Comment: 1s2p 3P1 energy has been calculated from the 1s2s 3P0 level using the NIST level separation. Thu Jul 20 13:42:29 2000 ...

res r . r , res r 0 0 , , 1 b­ , 2 1 exp a r 1. (1) . ... 6) erf (a ) . 2a 281 ( k 1) (k ) c 2a ( k ) e , (k ) 2 x0 erf a (k ) : , c 0.5 (0.9) , (0) 1 . ... 2 2 P1b P1F min ^ i ^ ^ 0 i 1 F T ^1i F 1 F T ^1i b , . ... min FT F 1 FTb . ... 1. , 0 1 156.25 147.74 150.0 154.95 s 2 1 ­ ­ ­ 19.3 -37.84 15.20 18.12 1019.3 880.55 840.5 961.29 11.4% 7.9% 14.8% 9.6% 282 0 0 ,0 0 0,02 0,04 0,06 0,08 0,10 0,12 0,14 0,16 -200 3 5 1 -400 (r), -600 4 -800 2 -1000 h= a-r, 1a 3.76 1 ­ 1 .; 4 ­ , res r ( 6 .; ...

... 2 I e = 8 ne a Te (1 + eqd aTe (e) c 2eqd = a 2 1 + me 2 a ) (i ) c 0, i* = 2 2 a (1 - 2eqd mi a ) , * i ni + i = 0 t i = nvi =- Di ni - ( Dne / Ti ) i ii exp exp eqd Ti a eqd - Ti - eq 1 noi exp - d 2 a 2Ti Ti li Ii = eqd Ti 2 1- 2 a Ti exp - 4 Deqd Ti a i 1 li - 1 , , I ph ( qd , a ) = a c 2 R + eqd a ( ) d ( ) = , 270 2c 3 exp -1 Tc 3 I ph ( qd , a ) = a c 2 1 R + eqd a ( ) d + 2 ( ) d 80 ­ ... Fluxus. ...

IEEE 2008 Nuclear Science Symposium, Meical Imaging Conference and 16th Room Temperature Semiconductor Detector Workshop , October 19-25, 2008 . Conference on the Design/Optimization of the Silicon Detector at the International Linear Collider , September 17-19, 2008 . LSC/Virgo Joint Meeting , March 17-20, 2008 . ...

Альтернативный форум . Scientific.ru Все форумы . ... Олег Баклан - 29.07.2006 21:37 . ... Пока сигнал долетит от одного зеркала к другому, пройдет время t1, и расстояние между зеркалами станет равным не Lo, a L1, где L1=Lo*exp(H*t1), в соответствии с законом расширения. ... Пока световой сигнал долетит от одного зеркала к другому пройдет время t2, и расстояние между зеркалами станет равным не L1, a L2, где L2=L1*exp(H*t2), в соответствии с законом расширения. ... tреал = tидеал*exp(Н*tидеал/2). ...