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81. IZMIRAN - Laboratory for ionosphere discontinuity investigation
... Main page . ... Main results . Data . ... webmaster@izmiran.ru . ... The main subject of the laboratory is investigation of the large-scale structure of the topside ionosphere. The researches are based on the vast bank of data of the Intercosmos-19, Cosmos-900, and Cosmos-1809 satellites. ... study of the large-scale inhomogeneous structure of the ionosphere, including the night-side and day-side main ionospheric trough, the day-side Muldrew trough, the ring ionospheric trough etc.; . ...
[ Сохраненная копия ]  Ссылки http://www.izmiran.rssi.ru/ionosphere/ionheterogeneity/index.shtml -- 7.9 Кб -- 09.04.2016
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82. The basic stages in the Earth's pre-geological development
... part 1 | ... The Basic Stages in Earth's Pre-geological Development . ... After fragments of the Vortex sleeves separated, whirlwinds of second and third orders ("NC" - new micro-vortex) were generated- future planet cores and their satellites - all of them developing independently, governed by the common laws of development of cosmogenic vortexes. ... Our planet's core today is comprised of considerably deteriorated cosmogenic vortex; consequently, the Earth has a moderated magnetic field. ...
[ Сохраненная копия ]  Ссылки http://www.lermus.ru/users/trunaev/part2.htm -- 22.6 Кб -- 04.12.2001
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83. http://solarwind.cosmos.ru/txt/2011/presentations/Sun/Ishkov/apj_691_2_1222.pdf
... Printed in the U.S.A. doi:10.1088/0004-637X/691/2/1222 AUTOMATED LASCO CME CATALOG FOR SOLAR CYCLE 23: ARE CMEs SCALE INVARIANT? ... CME RATE DURING CYCLE 23 Figure 2 shows the daily CACTus CME rate for cycle 23 in red, with the International Sunspot Number (e.g., Vanlommel et al. 2004) superimposed in gray as solar cycle reference. ... The CACTus CME speeds Figure 12. ... A comparison of a sample of common events shows that on average the CDAW CME width is wider than the CACTus CME width. ...
[ Текст ]  Ссылки http://solarwind.cosmos.ru/txt/2011/presentations/Sun/Ishkov/apj_691_2_1222.pdf -- 1208.5 Кб -- 15.04.2011
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84. Doclad, figures
. F IGURE . 4. Metallicity is plotted against galactocentric distance (a) and distance from the Galactic plane (b) for the globular clusters of thick disk (triangles) and old halo (circles). The slopes of linear regressions gives the values of radial and vertical metallicity gradients, corresponding. The points denoted with squares have been excluded from regressions according to the 3 rule. discussion in the text | previous figure | next figure .
[ Сохраненная копия ]  Ссылки http://ip.rsu.ru/~marsakov/conf/paper3/c3fg4.htm -- 2.2 Кб -- 02.02.2007
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85. http://www.abitu.ru/en2002/closed/viewwork.html?ext=175
... 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 { ...
[ Сохраненная копия ]  Ссылки http://www.abitu.ru/en2002/closed/viewwork.html?ext=175 -- 12.3 Кб -- 05.05.2006
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86. Izmccd
Download Izmccd (~2.7 MB). ... a) a choice of the best mode of measurements of stars and objects ("Properties/Measurement"), . b) a choice of reference stars. ... 1) necessity of presence on an image of a plenty of stars (we recommend to apply this mode, if on the frame of reference stars is more 100) . ... Sx and Sy depend from residuals at all reference stars (reference stars are marked by blue color). ... These residuals are the image of the star a minus function of a profile for each pixel. ...
[ Сохраненная копия ]  Ссылки http://www.izmccd.puldb.ru/izmccd4e.htm -- 7.6 Кб -- 17.09.2007
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87. УкрАстроФорум 2008 - стр. 1 - Астрономические мероприятия
... Астрономические мероприятия (Модераторы: mak , DF ) > . УкрАстроФорум 2008 . ... Мероприятия . ... Оффлайн . Сообщений: 1047 . Благодарностей: 19 . ... Рад сообщить вам, что подготовка Седьмого Всеукраинского Форума любителей астрономии "УкрАстроФорум 2008" вошла в свою активную стадию. ... Записан . ... Ответ #1 : 13 Февраль 2008, 17:56:20 ? Что ж, пусть и немного позже означенного срока, но тем не менее это свершилось: сегодня официально открыта регистрация на УкрАстроФорум 2008! ...
[ Сохраненная копия ]  Ссылки http://www.astroclub.kiev.ua/forum/index.php?topic=5324.0 -- 116.2 Кб -- 09.04.2016
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88. http://kcor.sai.msu.ru/arXiv1002.2360.pdf
... 000, 1­12 (2009) Printed 11 February 2010 A (MN L TEX style file v2.2) Analytical approximations of K -corrections in optical and near-infrared bands I1gor V. Chilingarian1 2 ,2,3 , Anne-Laure Melchior 1,4 and Ivan Yu. ... Received 2010 February 01; in original form 2009 August 14 ABSTRACT To compare photometric properties of galaxies at different redshifts, the fluxes need to be corrected for the changes of effective rest-frame wavelengths of filter bandpasses, called K -corrections. ... Table 1. ...
[ Текст ]  Ссылки http://kcor.sai.msu.ru/arXiv1002.2360.pdf -- 1631.3 Кб -- 12.02.2010
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89. astro-ph authors/title/abstract search for 'galaxy evolution ' all years
Title: Galaxy Deconstruction: Clues from Globular Clusters . ... Title: Environment and Galaxy Evolution at Intermediate Redshift . ... Title: Spectroscopic evolution of dusty starburst galaxies . ... Title: Early galaxy evolution from deep wide field star counts. ... Abstract abridged . ... Title: Cross-Roads in Studies of Galaxy Evolution . ... Title: Gas and Galaxy Evolution in Poor Groups of Galaxies . ... first 100 from a total of 158 matches for the search pattern galaxy evolution . ...
[ Сохраненная копия ]  Ссылки http://sed.sao.ru/lit/gal_evol1.html -- 91.9 Кб -- 15.07.2001
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90. New Page 11
... This is commonly referred to as CPM (cost per thousand impressions).We pay you a percentage of revenues for the ads that you and your friends view with Harry, based on current CPM rates.You will get 75% of total revenue generated from your viewing.. ... REMEMBER: for every one hour the program on Your screen You'll get paid $0.50. And when You recommend those program to Your friends, reffering to Your personal ID, You'll get paid $0.10 for every hour the program open on Your's friends computer. ...
[ Сохраненная копия ]  Ссылки http://sitilia.chat.ru/newpage11.htm -- 20.1 Кб -- 09.04.2016
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91. http://www.inasan.rssi.ru/~kurbatov/Kurbatov--2010phdt.nmceg.pdf
... 2010 2 1 1.1 1.2 1.3 1.4 1.5 . ... 30 2 2.1 2.2 2.3 2.4 2.5 2.6 . ... Interacting Galaxies , Koln, 12 7. ... OB-, , - 68 M = 10 0.3 [Fe/H] 0.2 6.5 Msol OB = 2 km/s 0.3 M = 10 6.5 Msol OB = 8 km/s 0.3 M = 10 7.5 Msol OB = 8 km/s 0.3 M = 10 8.5 Msol OB = 8 km/s [Fe/H] 0.2 0.2 [Fe/H] 0.2 [Fe/H] 0.1 0.1 0.1 0.1 0 - 2.5 0.3 [O/H] 0.2 -2 - 1.5 -1 - 0.5 0 0.5 0 - 2.5 0.3 [O/H] 0.2 -2 - 1.5 -1 - 0.5 0 0.5 0 - 2.5 0.3 [O/H] 0.2 -2 - 1.5 -1 - 0.5 0 0.5 0 - ... Vol. ...
[ Текст ]  Ссылки http://www.inasan.rssi.ru/~kurbatov/Kurbatov--2010phdt.nmceg.pdf -- 544.7 Кб -- 06.09.2012
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92. v21-2
... THE 'VON OPEL FLIGHTS' . ... Raab, with his partner Diploma Engineer Kurt Katzenstein would apply to their lightest aeroplane the solid-propellant Sander rockets that had proven themselves so well in Fritz von Opel's rocket cars. ... The von Opel-Sander-Stamer-Lippisch tests were elevated to a full-scale airplane immediately after the model flights ; in effect, this was to be the first manned rocket flight. ... FRITZ VON OPEL at the controls of the Opel Sander Rak. 1 rocket plane. ...
[ Сохраненная копия ]  Ссылки http://www.epizodsspace.narod.ru/bibl/spaceflight/21/opel.html -- 91.4 Кб -- 09.04.2016
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93. http://sun.sai.msu.ru/texts/somov-1-10Lect.pdf
Introduction to PLASMA ASTROPHYSICS (Selected 10 lectures) Boris V. Somov Astronomical Institute and Faculty of Physics Moscow State University Pushino-na-Oke, 2008 Contents Ab out These Lectures 1 Particles and Fields: Exact Self-Consistent Description 1.1 Liouville's theorem . . . . . . . . . . . . . . . . . . . 1.1.1 Continuity in phase space . . . . . . . . . 1.1.2 The character of particle interactions 1.1.3 The Lorentz force, gravity . . . . . . . . . 1.1.4 Collisional friction . . . . . . . . . . . .
[ Текст ]  Ссылки http://sun.sai.msu.ru/texts/somov-1-10Lect.pdf -- 1179.0 Кб -- 18.03.2014
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94. Deep Purple Discography
Shades of Deep Purple (USA: Tetragrammaton 1968 ; Europe: EMI Parlaphone 1968 ; Japan: Polydor 1968) (CD) . Deep Purple's debut album, recorded very hastily. ... Tracks: . ... Wring That Neck (Blackmore/Lord/Simper/Paice) . ... All tracks written by Blackmore/Gillan/Glover/Lord/Paice . ... Painted Horse (Blackmore/Gillan/Glover/Lord/Paice) . ... Child in Time (Live, 690924) (Blackmore/Gillan/Glover/Lord/Paice) . ... Bonus tracks on Japanese CD: Lazy (edited) (Blackmore/Gillan/Glover/Lord/Paice) . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/~util/dpd.html -- 36.7 Кб -- 01.10.2012
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95. http://www.2dfquasar.org/Papers/2002MNRAS.337..275C.pdf
... 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. ...
[ Текст ]  Ссылки http://www.2dfquasar.org/Papers/2002MNRAS.337..275C.pdf -- 831.9 Кб -- 04.03.2004
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96. http://www.astro-soc.odessa.ua/Program-2011.pdf
August, 2011, Odessa, Ukraine EVENTS: Monday, 22.08.2011 Arrival 09.00 ­ 22.00 Registration of participants 20.00 ­ 22.00 Evening session : , ( -), ( - «») Tuesday, 23.08.2011 06.05 09.00 09.00 11.00 13.00 13.15 14.30 15.50 16.20 18.00 19.00 19.55 21.00 06.06 09.00 11.00 11.30 13.00 14.30 16.30 18.30 19.53 ­ ­ ­ ­ ­ ­ ­ ­ ­ ­ 13.00 11.00 13.00 13.15 14.30 15.50 16.20 ... Discussion 6 SECTION SESSIONS Section 1. ... 15.50 - 16.20 Coffee break 16.20 - 18.00 Section sessions .. ...
[ Текст ]  Ссылки http://www.astro-soc.odessa.ua/Program-2011.pdf -- 575.3 Кб -- 23.07.2014
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97. 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 ...
[ Текст ]  Ссылки http://lukash.asc.rssi.ru/RADIOASTRON/MGJ0414+534/9708079/Table2.ps -- 71.8 Кб -- 06.05.2007
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98. http://uranus.sai.msu.ru/~seif/ST10_apj_722_586.pdf
... 1, 2010 Table 3 Best-fit Parameters of the Spectral Analysis of PCA and HEXTE Observation of SS 433 in 3­150 keV Energy Rangea Observational ID 10127-01-01-00 10127-01-02-00 10127-01-03-00 10127-01-04-00 10127-01-05-00 10127-01-06-00 10127-01 ... 1.39(1) 1.13(1) 0.99(1) 1.07(1) 0.98(4) 1.17(1) 1.15(3) 1.17(1) 1.21(3) 1.25(6) 1.06(2) 1.09(4) 1.23(1) 1.20(5) 1.07(7) log(A)b 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 ... Softening of X-ray spectra is seen when the Figure 2. ...
[ Текст ]  Ссылки http://uranus.sai.msu.ru/~seif/ST10_apj_722_586.pdf -- 1425.7 Кб -- 23.09.2010
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99. http://www.gpad.ac.ru/collaborations/gao/wv_solphys.pdf
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. ...
[ Текст ]  Ссылки http://www.gpad.ac.ru/collaborations/gao/wv_solphys.pdf -- 317.1 Кб -- 05.07.2006
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