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21. Six-Centimeter Radar Observations of 4179 Toutatis
... Old World First Asteroid Radar Echo. ... It testifies that 4179 Toutatis is a double object like asteroid 4769 Castalia. ... Interference of Radar Echo from the Binary Asteroid 4179 Toutatis. ... An analysis of the 6-cm radar data revealed quasi-harmonic oscillation of the echo’s “central” Doppler frequency with a period of about 14 sec and a deviation of about (0.7*B) Hz, where B is the echo bandwidth, which for 4179 Toutatis was equal to 2.1 Hz and 1.9 Hz for 1992 Dec 8 and 9, respectively. ...
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Ссылки http://www.cplire.ru/html/ra&sr/sr/4179-Toutatis/index.html -- 11.9 Кб -- 02.12.2002
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22. Juieshetye_diary
... Shetye,ѓЉJ. ; Kuridze,ѓЉD.; Henriques,ѓЉV.; Stangalini, M., Doyle,ѓЉJ.ѓЉG.; Scullion,ѓЉE.; Analysis of high--frequency transverse waves associated with movements of spicular--type events. ... Shetye,ѓЉJ. ; Doyle,ѓЉJ.ѓЉG.; Scullion,ѓЉE.; Nelson,ѓЉC.ѓЉJ.; Kuridze,ѓЉD.; Henriques,ѓЉV.; Woeger,ѓЉF.; Ray,ѓЉT. High-cadence observations of spicular-type events on the Sun. ... 3-2015) . ... NAM 2015 on High Cadence Observations and Analysis of Spicular-Type Events Using CRISP Onboard SST . ...
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Ссылки http://star.arm.ac.uk/~jus/publication.html -- 5.0 Кб -- 13.03.2016
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23. RCJ0311+0507
... A radio galaxy is a galaxy that emits an unusually big amount of energy at radio wavelengths. ... Inside of each galaxy with an active nucleus (radio galaxies are among them) there must be a system of a "central machine" responsible for the colossal amount of the emitted energy from radio to gamma ranges. ... Sometimes a radio source in an active galaxy may flare again if the needed conditions appear (a new portion of matter would fall into the furnace of the "central machine"). ...
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Ссылки http://www.sao.ru/Doc-en/SciNews/RC0311/ -- 7.8 Кб -- 01.10.2012
[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/RC0311/ -- 7.8 Кб -- 02.10.2012
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[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/RC0311/ -- 7.8 Кб -- 02.10.2012
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24. Two points (INTERBALL-1 and MAGION-4) observations of magnetopause motion
The close position of main satellite and subsatellite (distance between them about 1000 km) and using the similar sets of Faraday cups (VDP and VDP-S) with high resolution measurements (up to 16 Hz for the main satellite and up to 10 Hz for the subsatellite) allow us to determine the small-scale variations of the magnetopause shape and position and to estimate the velocity of the magnetopause motion. ... Two point observation of the magnetopause motion: the INTERBALL project. ...
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Ссылки http://www.iki.rssi.ru/tail/results/vdp/twopoint.html -- 4.2 Кб -- 03.01.1997
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/tail/results/vdp/twopoint.html -- 4.2 Кб -- 03.01.1997
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[ Сохраненная копия ] Ссылки http://www.cosmos.ru/tail/results/vdp/twopoint.html -- 4.2 Кб -- 03.01.1997
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25. Index
... Aloisi, A. The Old Stellar Population . Alonso-Herrero, A. HST /NICMOS Observations of the . ... Balcells, M. HST-NICMOS Observations of Galactic . ... Baum, S.A. Investigating the Evolution of . ... Becklin, E.E. A Coronagraphic Search for . ... Clampin, M. The Old Stellar Population . ... Close, L. HST NICMOS Observations of . ... The Stellar Population in . Geballe, T.R. HST NICMOS Observations of . ... Greggio, L. The Old Stellar Population . ... Leitherer, C. The Old Stellar Population . ...
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Ссылки http://www.stecf.org/conferences/sardinia/node40.html -- 14.1 Кб -- 12.06.2006
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26. Determination of the 'diffusion coefficient'.
Next: Determination of the stellar Up: Results. ... Their values taken from Lipunov (1992) are shown in table 1. ... For Vela X-1 and Her X-1 values of magnetic field, B , coincides with the values that we used when radii of NS's are and correspondently. ... Characteristic time for the wind-accreting systems can be determined from the equation: . ... These velocities are close to obtained using estimates of the 'diffusion coefficient'. These characteristic time scales are also shown in table 3. ...
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Ссылки http://xray.sai.msu.ru/~polar/html/publications/sissa065/node3.html -- 5.6 Кб -- 21.06.1996
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27. Semiclassical Microlocal Analysis (Fall 2003)
... Microlocal Analysis is a theory of Pseudo-Differential Operators and Fourier Integral Operators (PDOs and FIOs). ... Microlocal analysis comes in few flavors. ... We will consider semi-classical PDOs and FIOs: one can always get from there to standard PDOs and FIOs but semi-classical theory has more applications. Less formal description of (semi-classical) microlocal analysis is ``a semi-classical limit of quantum mechanics'' or ``high-frequency limit of electrodynamics'' (etc). ...
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Ссылки http://www.mccme.ru/ium/f03/microlocal.html -- 5.0 Кб -- 09.12.2005
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28. http://scan.sai.msu.ru/lk/
Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...
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29. RTT150 project data archive
RTT150 . ... HEAD IKI . This page is a search interface through RTT150 observationsdatabase which is stored at IKI. According to the agreement between participantsof RTT150 project, observational data fully belong to the institution which hascarried out this observation for one year, are available to all three partiesinvolved (IKI, KSU and TUG) during the second year and become freely accessibleto the whole astronomical community starting two years after observation date. ...
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Ссылки http://hea.iki.rssi.ru/AZT22/ENG/dbase.htm -- 7.0 Кб -- 18.02.2004
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30. HAEBE Clusters Analysis (Abstract)
... The large body of near infrared observations presented in Testi et al. (1997; 1998) are analysed with the aim of characterizing the young stellar clusters surrounding Herbig Ae/Be stars. The results confirm the tendency of early Be stars to be surrounded by dense clusters of lower mass "companions", while Ae stars are never found to be associated with conspicuous groups. ... Only the most massive stars (10-20Msun) are found to be associated with dense (10^3 pc^-3) stellar clusters. ...
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Ссылки http://www.arcetri.astro.it/~lt/preprints/haebe3/abstract.html -- 2.9 Кб -- 11.09.2007
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31. Celestial Mechanics
Subject of Celestial Mechanics. ... Differential Absolute Coordinates Equations of the Problem. ... General Integral of Non-Perturbed Motion. ... General Equation of Non-Perturbed Orbit. ... Other Integration Methods of Non-Perturbed Motion Differential Equations; Bine Equation for Case of Non-Perturbed Motion. ... Ellipsical Motion, Kepler Equation. ... Motion Differential Equations in Absolute Coordinates. ... Equation of System of Bodies Motion in Barycentric Coordinates, in Relative Coordinates. ...
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Ссылки http://space.univ.kiev.ua/courses/neb_mehan_e.html -- 5.0 Кб -- 23.02.2005
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32. FADPS - Flexible Astronomical Data Processing System
... The reduction system of observations FADPS (description in Russian) (Flexible Astronomical Data Processing System) for data of wide-band receivers of the first observation cabin of the radio telescope RATAN-600 had been created under the Unix-like operational system DEMOS for computers of the SM-1420-type (PDP/11) in 1987 for observation analysis and estimates of coordinates and flux densities of radio sources. ... FADPS: flexible astronomical data processing system at RATAN-600 in UNIX environment....
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Ссылки http://sed.sao.ru/~vo/fadps_e.html -- 15.4 Кб -- 24.02.2010
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33. http://www.wdcb.ru/stp/data/catal_Mirny/Catal_Mirny_Eng.doc
E.T. MATVEYEVA, R.V.Shchepetnov Сatalogue of geomagnetic pulsations of Pc1 type on observation data at the Antarctic Observatory Mirny Geophysical Observatory Borok, Institute of Physics of the Earth RAS, Russia The catalogue is based on the analysis of long-term and continuous observations of pulsations such as Pс1 on the Antarctic Observatory Mirny( ? ... C?- traces of Pc1. ... The period of Pc1 in seconds (Ts) is determinated as averaged prevailing in the given time interval. ...
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Ссылки http://www.wdcb.ru/stp/data/catal_Mirny/Catal_Mirny_Eng.doc -- 32.0 Кб -- 18.01.2010
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34. http://www.asc.rssi.ru/RadioAstron/meetings/telecon/oct10_2011.pdf
... VLBA+Italy survey (to contact the schedulers) (closed) E.Fomalont and J.Romney: To provide some review of problems happened with fringe search in VSOP project. (closed) M.Popov : To compose a tentative time -table of possible observations , and inform the observatories on the specific time slots that might be requested for fringe search program in October-November. (continued) C. Gwinn: to try to compile FAKERAT software on modern platforms. (closed) GBT and ...
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Ссылки http://www.asc.rssi.ru/RadioAstron/meetings/telecon/oct10_2011.pdf -- 41.0 Кб -- 13.12.2011
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35. http://lukash.asc.rssi.ru/RADIOASTRON/MGJ0414+534/9708079/Table2.ps
... Julian Date Flux Densities (mJy) Julian Date Flux Densities (mJy) 2440000:0 A1 A2 B C 2440000:0 A1 A2 B C 8930.9968 153.8 134.6 59.8 22.6 9021.6846 154.0 137.0 59.0 22.9 8939.7717 163.7 146.0 66.1 22.9 9024.6766 151.4 134.6 58.4 22.1 8940.8936 153.2 135.8 59.2 22.6 9030.5334 156.7 139.1 59.0 22.4 8944.7380 161.7 142.2 63.7 23.1 9032.6650 151.8 136.5 57.7 22.6 8951.8637 148.4 131.3 58.3 21.7 9036.7067 155.1 137.1 58.8 ...
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Ссылки http://lukash.asc.rssi.ru/RADIOASTRON/MGJ0414+534/9708079/Table2.ps -- 71.8 Кб -- 06.05.2007
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36. http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt_meteors.pdf
To appear in "Fourth Workshop on Robotic Autonomous Observatories (2015)"RevMexAA(SC) METEOR OBSERVATIONS WITH MINI-MEGATORTORA WIDE-FIELD MONITORING SYSTEM S. Karpov, 1, 3 N. Orekhova2 G. Beskin, 1, 3 A. Biryukov3,4 S. Bondar,2 E. Ivanov,2 E. Katkova,2 A. Perkov, and V. Sasyuk3 RESUMEN 2 Favor de prop orcionar un resumen en espanol. ... The faintest detected meteors has the peak brightness about 10 mag, while the ma jority - from 4 to 8 mag. ... 2010; Karpov et al. 2013; Beskin et al. ...
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Ссылки http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt_meteors.pdf -- 115.6 Кб -- 15.12.2015
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37. Courses
... Exams . Mathematical Analysis . ... Mechanics . ... Methods of Processing Observation . Tests . ... Mathematical Analisis . ... Theory of Functions of Complex Variables . Probability Theory and Mathematical Statistics . ... Mathematical Methods in Physics . Atomic Physics and Spectroscopy . Electrodynamics and Theory of Radiation . Theoretical Mechanics . ... Quantum Mechanics . ... Course of Specialization . ... Complementary course . Nuclear Physics . ...
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Ссылки http://comet.sai.msu.ru/astrodiv/plan.html -- 4.3 Кб -- 27.10.1997
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38. SN1989B in M66
... In the light curve depicting their observations, definite trends are noted, here is a "thumb-nail" analysis of the the magnitude estimations of the bright SN (1989B) in the galaxy NGC 3627 (M66). ... 10 (IAUC # 4742) 2/25 13.3 16 j 2/27 13.5(*) 18 lc 2/28 13.8 19 p 3/1 13.2 20 w 3/2 13.5 21 a 3/4 13.8 23 p 3/6 13.3 25 c 3/7 13.3 26 c 3/8 14.1 27 m 3/8 13.3 27 r 3/9 13.4 28 c 3/9 14.1 28 m 3/10 13.6 29 j 3/10 14.0 29 a 3/11 13.6 30 c 3/11 13.5 30 r 3/11 13.7 30 s 3/13 [13.69 CCD Mag.] ...
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Ссылки http://www.sai.msu.su/mirrors/isn/snimages/sn1989b.html -- 9.7 Кб -- 22.12.2007
[ Сохраненная копия ] Ссылки http://www.rochesterastronomy.org/SNIMAGES/sn1989b.html -- 9.7 Кб -- 10.04.2016
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39. Igor V.Kukushkin
... He pioneered investigation of the two-dimensional electron energy spectrum under the conditions of the quantum Hall effect and discovered the magnetooptical manifestation of the fractional quantum Hall effect observed as a spectral step of two-dimensional electron recombination lines. ... In 1990 these achievements were summarized by I.V.Kukushkin in his DPhil thesis Magetooptics of Two-Dimensional Electrons under the Conditions of the Fractional Quantum Hall Effect and Wigner Crystallization. ...
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Ссылки http://www.issp.ac.ru/engl/rasmembers/37-igor-vkukushkin -- 19.1 Кб -- 10.04.2016
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40. Plasmoids [Oulu]
spaceweb@oulu.fi - last update: 27 November 1998, 1900 UT (RR) . Tailward fast plasma flows with dipolar Bz signatures (north-then-south turning of B) observed within plasma sheet are called plasmoids (e.g., Hones et al., ... Most plasmoids have also helical magnetic field structures (large By fields), called "flux ropes" (Hughes and Sibeck, 1987; Slavin et al., ... 1998). ... Observations of plasmoids are highly correlated with substorm onsets (Moldwin and Hughes, 1993; Nagai et al., ... Lett. ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/SPPHTEXT/substorms/plasmoids.html -- 4.9 Кб -- 21.12.2007
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Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
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