... 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.; . ...

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• IZMIRAN - Laboratory for Physics and modeling of the ionosphere
• POLAR 2013

... 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. ...

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... 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. ...

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. 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 .

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• Population of Galactic globular clusters, figures
• RR LYRAE VARIABLES SUBSYSTEMS IN THE GALAXY, figures

... 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 { ...

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• http://www.abitu.ru/en2002/closed/viewwork.html?work=150

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. ...

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... 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! ...

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... 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. ...

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• http://kcor.sai.msu.ru/arXiv1102.1159.pdf

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 . ...

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• astro-ph abstracts (body) search for 'photometric redshifts' all years

... 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. ...

91. http://www.inasan.rssi.ru/~kurbatov/Kurbatov--2010phdt.nmceg.pdf

92. v21-2