... Проф. А.Д.Чернин (ГАИШ, МГУ, Москва): ЭНЕРГЕТИЧЕСКИЙ СОСТАВ ВСЕЛЕННОЙ: НОВАЯ СИММЕТРИЯ 13.00-15.00. ... Проф. Л.И.Мирошниченко (ИЗМИРАН, Троицк, Россия): СОЛНЕЧНОЗЕМНЫЕ СВЯЗИ В 23-ЕМ ЦИКЛЕ СОЛНЕЧНОЙ АКТИВНОСТИ Лекция 9 10.50-11.30. ... М.И.Рябов, А.Л.Сухарев (Одесская обсерватория Радиоастрономического института НАНУ) : О ПРОЯ ВЛЕНИИ ИЗМЕНЕНИЙ СТРУКТУРЫ ПЕРЕМЕННО СТИ ПОТОКОВ ВНЕГАЛАКТИЧЕСКИХ РАДИОИСТОЧНИКОВ 3С120, OJ287, 3С273, 3С279, 3С454.3 НА РАЗЛИЧНЫХ ФАЗАХ АКТИВНОСТИ 4. ... РИ НАНУ Гравиметр. ...
Computer Ephemeris for 2014 from DE200/LE200. Reduction quantities ( dynamical time scale). tau A+A' B+B' C D E A' B' a 0s0001 0 001 0 001 Jan 1 -0.5000 -5.888 8.279 -3.493 20.488 14 16 88 2 -0.4973 -5.772 8.253 -3.823 20.418 14 63 65 3 -0.4945 -5.674 8.209 -4.152 20 tau A+A' B+B' C D E A' B' a 0s0001 0 001 0 001 Feb 1 -0.4151 -3.903 7.810 -12.669 15.552 15 88 -44 2 -0.4124 -3.876 7.764 -12.915 15.304 15 63 -74 3 -0.4097 -3.860 7.739 -13.157 ...
... If you have the option, run the scheduler in a way that the visit(s) are biased toward the areas where the resources are below the limit lines (particularly for the total orbits, SAA-free orbits, and SAA-hider orbits ). ... From the LISP/SPIKE command line. ... Below are several examples of how to run the scheduler from the command line. ... It will select any visit which doesn't have plan windows and is lrp_state=ready or visits which are missing their constraints and run the scheduler on them. ...
... Moreover, it even seems at all doubtful that solar wind velocity variations be mainly determined by the field structure in the Sun. ... The solar wind velocity values, V,, obtained by Wang and Sheeley (1990) from the expansion factor, f,, are: V, 650 km/s 650 km/s 2 V, 550 km/s 550 km/s 2 V, 450 km/s 450 km/s 2 V, f, 3.5 3.5 5 9.0 9.0 5 f, 18.0 fJ 18.0 _ f, THE SOLAR WIND PARAMETERS The histopam of relation between the measured velocities and the velocities Table 1...
... One year of Kepler observations of KIC 1718290 reveals a rich spectrum of low-amplitude modes with periods between 1 and 12 hr, most of which follow a regular spacing of 276.3 s. This mode structure strongly resembles that of the V1093 Her pulsators, with only a slight shift toward longer periods. ... Key words: stars: horizontal-branch stars: individual (KIC 1718290) stars: oscillations stars: variables: general subdwarfs Online-only material: color figures 1. ...
... Total time in scheduled scans: 8.91 hours. ... Total number of baseline hours: 8.91 (Recording scans only) Projected maximum data output rate from the correlator: 8.2 kbytes/sec if processed in one pass. ... Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) * F219023 18 11 22.097728 * 18 14 32.287000 18 14 58.395312 0.00 -28 37 42.43897 *-28 36 45.82800 -28 36 48.07173 0.00 From catalog imbedded in main SCHED input file. 0.083 scan hours, 0.000 baseline hours above horizon. ...
... Optical Identifications X ray Optical Survey Name S 0:5\Gamma2 keV RA (J2000) Dec ` RA (J2000) Dec O\GammaX E O O\GammaE ID z Notes erg s \Gamma1 cm \Gamma2 h m s ffi 0 00 0 h m s ffi 0 00 00 CRSS0007.3+2042 0.48\ Theta10 \ Gamma13 00 07 21.9 +20 42 04 13.6 00 07 21.7 +20 42 02 2.6 18.53 18.78 0.24 QSO 0.7686 CRSS0007.5+2034 0.34\ Theta10 \ ... The closest optical counterpart is a faint source with an ambiguous optical spectrum. ...
EUROPEAN ORGANISATION FOR NUCLEAR RESEARCH CERN-EP-2000-148 OPAL PR 328 30 Novemb er 2000 Precise Determination of the Z Resonance Parameters at LEP: "Zedometry" The OPAL Collaboration Abstract This final analysis of hadronic and leptonic cross-sections and of leptonic forward-backward asymmetries in e+ e- collisions with the OPAL detector makes use of the full LEP 1 data sample comprising 161 pb-1 of integrated luminosity and 4.5 Ч 106 selected Z decays. An interpretation of the data in terms of
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