... 24 } Line { SrcBlock sin SrcPort 1 DstBlock func1 DstPort 1 } Line { SrcBlock Fcn SrcPort 1 Points [0, -55] DstBlock func DstPort 1 } Line { SrcBlock (G*M) ^1/2 SrcPort 1 Points [25, 0] DstBlock func DstPort 3 } Line { SrcBlock func SrcPort 1 Points [40, 0] Branch { ...

See also: Name-based Virtual Hosts Support . As the term IP-based indicates, the server must have a different IP address for each IP-based virtual host . ... There are two ways of configuring apache to support multiple hosts. ... For each installation, use the Listen directive in the configuration file to select which IP address (or virtual host) that daemon services. e.g. Listen www.smallco.com:80 It is recommended that you use an IP address instead of a hostname (see DNS caveats ). ...

... Родился 9 ноября 1958 года в городе Миннеаполис (Minneapolis), штат Миннесота (Minnesota), но родным считает город Салина (Salina) в штате Канзаз (Kansas). ... С 1993 по февраль 1996 года работал летчиком-испытателем в Космическом центре НАСА имени Джонсона (NASA Johnson Space Center). ... Ушел в отставку в 1993 году. ... Был одним из 106 кандидатов в астронавты, финалистов 13-го набора НАСА 1990 года, вызванных в Космический центр им.Джонсона на недельное медицинское обследование и собеседование. ...

... 337, 275­292 (2002) The correlation of line strength with luminosity and redshift from composite quasi-stellar object spectra S. M. Croom,1 K. Rhook,1 E. A. Corbett,1 B. J. Boyle,1 H. Netzer,2 N. S. Loaring,3 L ... We measure highly significant Baldwin effects for most broad emission lines (C IV 1549, C III] 1909, Mg II 2798, H ,H ) and show that they are predominantly caused by correlations with luminosity, not redshift. ... The correlations of log W with log(1 + z ) for each line. ...

... Миссия "Cassini - Huygens" (NASA и ESA) . ... Хронология за 2004-2006 года . ... Close (altitude = 2,100 km; 1,300 mi) of moon . ... Distant (altitude = 68,000 km; 42,000 mi) of moon . ... Cassini passage through plane [South to North] (160,000 km; 100,000 mi wrt ) . ... Closest distance (78,000 km; 49,000 mi) to on rev number 0 . ... Distant (altitude = 107,000 km; 67,000 mi) of moon . ... 01/03/2005 . ... Closest distance (211,000 km; 131,000 mi) to on rev number 3 . ... Start rev number 3. ...

... Pourquoi les constantes universelles ont-elles des valeurs si particuliцЁres ? ... Loin de jouer les mouches du coche, les ц©nigmes sont un moteur et un ц©lan pour l'astronomie et la physique car elles nous projettent au-delц  de ce qui est aujourd'hui pensable scientifiquement ou testable techniquement. Tout comme les thц©ories d'aujourd'hui se sont bцўties sur les mystцЁres d'hier, les ц©nigmes actuelles sont les clins d'е“il des thц©ories futures. ... Y a-t-il une thц©orie du Tout ?) ...

Хранение ультрахолодных нейтронов в магнитной ловушке из постоянных магнитов. ... Прецизионное измерение времени жизни свободного нейтрона (n в экспериментах при низких энергиях имеет принципиальное значение для физики элементарных частиц и космологии. ... Для используемой геометрии ловушки для эффективной очистки спектра через нижний барьер требуется не менее 400 с. Использование магнитного хранения УХН для измерения времени жизни нейтрона имеет одну замечательную особенность. ...

... Russian Academy of Sciences, . Sibirian Department, Yakutsk Scientific Center . Directors: Germogen F. Krymsky, Director, corresponding member of Russian Academy of Sciences . Evgeny G. Berezhko, Deputy Director . ... The main scientific directions are physics and astrophysics of cosmic rays, physics of solar-terrestrial interactions, investigations of interplanetary and near-the-Earth space, physical processes in magnetosphere and ionosfhere of the Earth. ...

... 35, No. 2, pp. 87­99. i Star Formation History in the Central Region of the Barred Galaxy NGC 4245 O. K. Sil'chenko1* , I. V. Chilingarian1, 2 , and V. L. Afanasiev 1 2 3 Sternberg Astronomical Institute, Universitetskii pr. ... The galaxy has been found to possess a pronounced chemically decoupled compact stellar nucleus, which is at least a factor of 2.5 richer in metals than the stellar population of the bulge, and a ring of young stars with a radius of 300 pc. ... NGC 4245. ...

... The draft classification (version August 9, 2006) for new GCVS versions . IAU XXVIth General Assembly, . ... Along with the "+" sign (coexistence of two types), it is suggested to introduce the "|" sign (meaning "or") – for classification options for the same object, e.g. EC|Ell, EC|RR. Pulsating variables . Present: . ... L, Lb (for red stars) . ... Eruptive variables . ... Move to rotating variables . ... ACV, SXARI . ACV . ... Cataclysmic variables and other stars with outbursts . ...

... The OC "MIr" and the cargo ship operations scheduled for 20-21 Feb. complete. The onboard systems of the Station and the cargo ship checked out, the orbit monitoring performed. The Station remains pressurized, the onboard systems perform norminal. ... The current flight of the Orbital Complex "MIR" is under constant control of TsUp and Ground Command complex. The OC "Mir" and the cargo ship onboard systems check out and the orbit monitoring are scheduled for 21-22 feb 2001. ...

... Like many other Western industrialized cities, London has experienced an absolute population decline in the central city, with people moving out to the suburbs. ... In 1988, for example, nearly 1 in 8 people were unemployed throughout London and the situation in the inner city was worst. ... More successful has been the government's attempt to encourage grwoth outside London without allowing the city to sprawl into umanageable suburban growth. ...

... Contacting and discussing with people sharing your interests, participating in night sky observations with telescopes as well as a large choice of astronomical books, magazines and video-tapes out of our club library. ... The seasons, the seeing ( a clear sky is not always associated to calm , stable air ) and most important how dark your observation site is. ... Therefore a dark site for observing is at least as important for deep sky observation as the diameter of your scope. ...

... Direct data transmission rate (Mbps) . ... the density of electron fluexs with energies in four bands from 0.04 MeV to 1.7 MeV; . ... sensor (TV, IR) data and heliogeophisical information (HGI) transmission to data receiving and processing centers at a rate of up to 2.56 Mbps; . ... 1.76 GHz - TV- and heliogeophysical information and DCLI's data transmission to data receiving and processing centers; . 7.5 GHz - TV- and heliogeophisical data transmission to data receiving and processing centers; . ...

Maria M. Katsova . I am a Leading Researcher in Stellar Astrophysics Department of SAI MSU . I began to work at Sternberg Astronomical Institute (SAI) in 1967, graduated from Moscow State University (MSU) in 1971, Ph.D.(MSU) since 1984. And now I become a Doctor of Sciences (Full Doctor of the Physical and Mathematical Sciences)(MSU, since 1999). ... I am a member of European Astronomical Society (EAS), Euro-Asian Astronomical Society (EAAS), National Geographic Society (NGS). ...

V.K.Gusev, A.V.Dech, G.A.Gavrilov, V.E. Golant, S.V.Krikunov, R.G.Levin, V.B.Minaev, E.E.Mukhin, A.N.Novokhatskii, Yu.V.Petrov, N.V.Sakharov, . A.F. Ioffe Physico-Technical Institute, Russian Academy of Science, St. Petersburg, Russia . T.A.Burtseva, A.B.Mineev, E.N.Rumyantsev . D.V. Efremov Institute of Electrophysical Apparatus, St. Petersburg, Russia . ... St. Petersburg, Russia . ... Institute of Physical Chemistry, Moscow, Russia . Last updated Wednesday, 3 Octomber, 2012 . ...