... The OC "Mir" orbit parametres before the final burns . ... Orbit period (in min) . ... Mean orbit altitude (km) . ... solar F 10.7 flux . ... F 10.7 <= 100 - low level; 100 < F 10.7 < 150 - medium level; F 10.7 >= 150 - high level . Orbit 86328(15) - the first burn bulding the descent orbit  D V 1 =9.3 m/s. After burn altitude H min = 188.2 km, H max = 219.2 km. Orbit 86329(16) - the descent orbit second impulse D V 2 =10.4 m/s. After burn altitude H min = 158.9 km, H max = 218.5 km. ...

... All circuit parameters have been presented in a symbolic form. ... To use the program you will need a CIR file (PSpise, DesignLab file) of your circuit. CIR file examples have been enclosured: bpasside.cir, test1.cir, test2.cir, test3.cir, test4.cir, laksamp.cir, bridge.cir, uA741acf.cir, quartz.cir. ... Ideal operational amplifier (nullor) * Nname n1 n2 n3 n4 * * In the ideal op amp data, (n1,n2) represent output nodes, * (n3,n4) represent input nodes (noninverting, inverting). ...

Olga V. Kochina . ... Russia, Moscow, 119017, . ... Modeling the synthesis of complex molecules in protostellar objects', Kochina O. V., Wiebe D. S., Vasyunin A. I., 2012, Physics of the Universe, Conference for young scientists, Ekaterinburg, Russia . Modeling of the formation of complex molecules in protostellar objects', Kochina O. V., Wiebe D. S., Kalenskii S.V., Vasyunin A. I.,2013 Astronomy Reports, Vol. 57(11), pp: 818 - 832 . ... Ultraviolet Universe - 2010", Saint-Petersburg, Russia. ...

... Высокоточные положения спутников Юпитера, Сатурна и Урана из 20 - летних пулковских наблюдений как основа для построения и уточнения современных теорий движения спутников планет. ... Все результаты наблюдений включены в Астрометрические базы данных Пулковской обсерватории (II база, http://www.puldb.ru) и могут использоваться для построения и улучшения теорий движения спутников планет. ... Результаты астрометрических наблюдений галилеевых спутников Юпитера в Пулковской обсерватории в 1986-2005 гг./ ...

... ---------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- catalog .dat 269 36020 Revised NLTT Catalogue and 1st Supplement Description of catalog columns (see Paper II for details): -------------------------------------------------------------------------------- Summary Information 1) NLTT number (drawn consecutively from 1 to 58,845) 2) binary component 3) RA ( 2000 ), epoch 2000 ( ...

... It is consonant with the wording of Isaiah speaking of the 'Hidden God' hidden even in the beginning of the universe .. ... Georges Lemeiter / . If the world has begun with a single quantum, the notions of space and would altogether fail to have any meaning at the beginning; they would only begin to have a sensible meaning when the original quantum had been divided into a sufficient number of quanta. ... Жорж Леметр , Бельгийский католический священник, астроном и математик. ... Путин [28] . ...

... 322, L29 ± L36 (2001) The 2dF QSO Redshift Survey ± V. The 10k catalogue S. M. Croom,1w R. J. Smith,2 B. J. Boyle,1 T. Shanks,3 N. S. Loaring,4 L. Miller4 and I. J. Lewis1 1 2 3 4 Anglo-Australian Observatory, PO Box 296, Epping, NSW 1710, Australia Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead CH41 1LD Department of Physics, University of Durham, South Road, Durham DH1 3LE Department of Physics, Oxford University, 1 Keble Road, Oxford OX1 3RH Accepted 2001 March 7....

... 2014 . ... MAGNETIC FIELDS IN SOLAR ACTIVE REGIONS V.G.Lozitsky Taras Shevchenko National University of Kyiv, Astronomical Observatory lozitsky@observ.univ.kiev.ua, lozitsky_v@ukr.net Magnetic field measurements in solar active regions carry out on a base of the Zeeman effect. ... TRACKING OF RADIO BURST SOURCES IN SOLAR CORONA BY HELIOGRAPHIC MEANS Koval A.A. 1, Stanislavsky A.A. 1,2, Konovalenko A.A. 1 Institute of Radio Astronomy of NAS of Ukraine 2 V.N. Karazin Kharkiv National University 1 .. ...

... The recurrent bipolar pores were observed at the middle latitudes of the Southern hemisphere since 27.04 to 7.05. ... The fine bipolar sunspots were observed at the middle latitudes of the Northern hemisphere since 31.05 to 5.06. ... The fine bipolar sunspots were observed at the middle latitudes of the Northern hemisphere since 24.06 to 28.06, in the Western part of the Sun disc. ... The fine bipolar sunspots were observed since 18.07 to 25.07 at the 25th parallel of the Northern hemisphere. ...

... Maps of six sources (0420+022, 0420-014, 1308+326, 1345+125, 1803+784, and DA 193) obtained with milliarcsecond resolution are presented and discussed, together with their broadband (1­22 GHz) spectra obtained on the RATAN­600 radio telescope at epochs close to those of the VLBI observations. ... The image (Fig. 5) shows that the source structure at 18 cm is compact, consisting of a VLBI core and two jet components, with the outer component lying 5 mas (30 pc) to the northwest of the core ( = 54 ). ...