... nlayc***solvefinishc***c*** Enter post processor and calculate the variance of the error weightedc*** with area.c***/post1setnsel,s, node ,,44fsum* get ,f01,fsum,fynsel,s, node ,,77fsum* get ,f02,fsum,fynallf01=-f01f02=-f02c*** aa00 = -1.468e-003 aa02 = -3.104e-006 aa04 = -4.111e-010 aa06 = 1.377e-015 c*** ab00 = 35.881ab02 = -0.00073173ab04 = 1.3682e-08ab06 = -4.0372e-14c*** vsum =0.0wsum=0.0* get ,y1, node ,528,u,yy1=( ...

October 17, 2010 ================ CDK125 and Nikon D3s Exposure of 0.001 seconds at ISO 1600 nikon_1287376892_moon_0p001s_1600iso.jpg was taken at Wed, 30 Jan 1974 00:28:09 GMT You can convert any unix time stamp to GMT (UTC) at this website: http://www.onlineconversion.com/unix_time.htm

Impact ­ Produced Exosphere of Europa A.A. Berezhnoy Sternberg Astronomical Institute, Moscow, Russia Equilibrium chemical composition of the impact-induced cloud 0.5 0.45 0.4 0.35 0.3 0.25 0.2 0.15 0.1 3000 3500 4000 T, K 4500 OH H2 5000 O 5500 H H2O Q 0.0045 0.004 0.0035 0.003 0.0025 0.002 0.0015 0.001 0.0005 0 2000 Na NaO H NaO 3000 T, K 4000 5000 1.E-01 2000 Q 1.E-02 1.E-03 1.E-04 T, K 2500 CO 3000 ... Previous detection of cometary impacts on Europa is very tentative. ...

... TRF - TRS. ITRS ITRF. ... TRS 1 TRS 2 X ( 2) = T1, 2 + 1, 2 R1, 2 X (1) IERS, ITRF2000 ITRF2005 Transformation parameters at epoch 2000.0 and their rates from ITRF2005 to ITRF2000 (ITRF2000 minus ITRF2005) T T T D 10 -9 1 2 3 R 1 R 2 R 3 mm 0.1 ± Rates ± 0.3 -0.2 0.3 mm - 0.8 0.3 0.1 0.3 mm - 5.8 0.3 -1.8 0.3 mas 0.000 0.012 mas 0.000 0.012 mas 0.000 0.012 0.40 0.05 0.08 0.05 0.000 0.000 0.000 0.012 0.012 0.012 (ITRF ) 20 40 2 10 ­9 12 ( ) 3-5 4- 20 3-8 25-30 1 / 1-3 / 10 / x, y z : (c...) : (c... ...

... Data It is now clear that fuzzballs are actually galaxies. ... Using the automatic telescope, we measured the redshifts and brightnesses of a large number of fuzzballs in all regions of the sky. ... Correlation between brightness and redshift Redshifts and Brightnesses 0.005 0.004 0.003 0.002 0.001 0 -0.001 0 -0.002 -0.003 -0.004 -0.005 Redshift of Fuzzball 500 1000 1500 2000 Brightness of Fuzzball The brightnesses and redshifts of all the fuzzballs measured are shown in this graph. ...

... SWXCS J000315-5255.2 . ... SWXCS J000324-5253.8 . ... SWXCS J002437-5803.9 . ... SWXCS J005500-3852.4 . ... SWXCS J011432-4828.6 . ... SWXCS J021705-5014.2 . ... SWXCS J021747-5003.4 . ... SWXCS J023924-2505.1 . ... SWXCS J035259-0043.7 . ... SWXCS J044144-1115.6 . ... SWXCS J062155-6228.6 . ... SWXCS J082113+3200.1 . ... SWXCS J084749+1331.7 . ... SWXCS J085524+1102.0 . ... SWXCS J090946+4157.2 . ... SWXCS J092729+3010.8 . ... SWXCS J092650+3013.8 . ... SWXCS J092719+3013.7 . ...

... Глава 2 . ... Ссылка из Главы 4 ). ... 4.3 . ...

... 268, 274), ( P , 680, 710)) OSF_flat_pr=( ( n , 0, 10), ( T , 250, 285), ( P , 500, 750)) def applyPriors(obsmod, prior = None , log_pr= False ): Apply prior information to a model -- supports flat or log-flat priors : param obsmod: The base model : param prior : List of lists defining the prior ranges : param log_pr: If true, use log-priors if prior is ... If None assume pointing straight up :param sampler: Allow different samplers to be run. ...

ISSN 1561 8889. . 2009. . ... 1 2 3 3 i , , ESTEC, () « », , ARTEMIS ESA ( 7.2°) 70 . ... ARTEMIS OGS ESA [4, 8]. ... M = m [r a ] , M h = mh [rh a h ] , (2) (3) J = (r0)2 m , Jh = (r0h)2 mh , ISSN 1561 8889. ... Performance of satellite to ground communications link between ARTEMIS and the Optical Ground Station // Proc. SPIE. ... Investigation of Atmospheric Instability for Communication Experiments with ESA's Geostationary Satellite ARTEMIS // Kine matics and Physics of Celestial Bodies. ...

... Горизонты науки о Вселенной (Модераторы: Дмитрий Вибе , AlAn ) ? Давайте приколем инопланетян! :) . ... Рейтинг: +0/-0 . ... 19.05.2005 [11:05:30] ? ... Ин