... 23 Algorithm fo r evalua tion of two burn maneuv ers using linearity Input information: ( t t E1 , rEI , v t1L , t E2 2L ( ) EI )T )T ­ ­ ­ ­ the time and the state vector of initial orbit for this time ; interval of possible thrusts for transition from initial orbit to the transfer on e; the time and the state vector of the target orbit for this time ; ... We cal culate the state vector for the initial orbit for the time t1a and the target one ­ for the time t2 a . ...

MUON METHOD FOR A MATTER STUDYING Yu. ... З МТЪУflВВ , ВПfl ПУММњИ ПВЪУ Оfl ЩЛБЛНЛ Л iЛПЛЛ НУМВМТЛУ,ММњi Л ,,БУУћ БМњi ЩБ ЛПВВЪ ЪНУВ КВ БМ~ВМЛВ, НН ПВЪУ flВ МУ,,У П,,МЛЪМУ,,У ВБУММТ ЛОЛ ПfiТТћЫУ,ТНfl ,,ПП-ТФВНЪ УТНУФЛfl. ы. е. ЕЦгймлйЗ, З. и. леагЙД еУТНУ,ТНЛИ ЩЛБЛНУ-ЪВiМЛ~ВТНЛИ ЛМТЪЛЪЫЪ, СУО,,УФ ЫМњИ еУТНУ,ТНУИ УћО. ЗЗЦСЦзаЦ 76 ї ЕВОУЫТУ, ы.е., лПЛО,, З.и., 1999 : ( ), , , чSR-, , . чSR . ... ЕЦгймлйЗ ы.е., леагЙД З.и. унй нДдйЦ еыйззхв еЦнйС аллгЦСйЗДзаь ЗЦфЦлнЗД 77 M mr. : . ... 3) : cos | ...

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... 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 .. ...

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Solar Physics (2006) 233: 89-106 DOI: 10.1007/s11207-006-2850-y C Springer 2006 ON THE POSSIBLE CONNECTION BETWEEN PHOTOSPHERIC 5-MIN OSCILLATION AND SOLAR FLARE MICROWAVE EMISSION A. G. KISLYAKOV and V. V. ZAITSEV Institute of Applied Physics, Nizhny Novgorod, Russia (e-mails: agkis@appl.sci-nnov.ru; za130 Dynamic spectra of low-frequency modulation of microwave emission from solar flares are obtained. ... PHOTOSPHERIC 5-MIN OSCILLATION AND SOLAR FLARE MICROWAVE EMISSION 93 Figure 2. ...

M obile A stronomical Sy stem of TE lescope- R obots MASTER-II Kislovodsk Lomonosov Moscow State University, Sternberg Astronomical Institute , Moscow Union "Optic" , Kislovodsk Solar Station Latitude = 43 o љ44'.767љN; Longitude = 42 o љ31'.417љE; Altitude = 2067љm MASTERљIIљ(8љsquareљdegress) + MASTERљVWF(VeryљWideљFieldљCameras (FOV=800 square degrees, Timeљresolutionљupљtoљ150љms, with unfiltered m_lim=14m on 5 sec. exposure, and ~10.5m with 0.15 sec) . ... 11h 38m 38.0s , -09d 59m 59s) . ...