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41. HIGH RESOLUTION IONOSPHERIC MASS SPECTROMETER P-11
HIGH RESOLUTION IONOSPHERIC MASS SPECTROMETER P-11 . ... Onboard mass-spectrometric equipment for study of neutral and ionized components of Earth upper atmosphere. Mass-spectrometer P-11 is one of P-series modifications of the on board radio-frequency monopole spectrometers. ... The instruments of P-series have passed successful approbation in space experiments aboard geophysical rockets MP-12, launched for investigation of Earth upper atmosphere (Ref. ... Measured mass number range, AMU - 1.. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/projects/warning/p-11.html -- 5.7 Кб -- 15.02.2000
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42. Laboratory of spectroscopy of defect structures ISSP RAS
... For SIMS (Secondary Ion Mass Spectrometry) analysis, a solid surface is bombarded by primary ions of some keV energy. ... The subsequent mass analysis of the emitted ions provides detailed information on the elemental and molecular composition of the surface. ... Extremely short ion pulses with a duration below . ... By rastering a fine-focussed ion beam over the surface, like an electron beam in an electron microprobe, mass resolved secondary ion images (chemical maps) can be obtained...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/lsds/en/methods/sims.html -- 10.6 Кб -- 10.04.2016
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43. Scientific.ru Альтернативный форум
Альтернативный форум . Scientific.ru Все форумы . ... Александр Тимофеев - 21.02.2006 17:23 . ... M_Europa=4.80e22 . ... Пусть теперь Уважаемый Пинопа потрудится дать "теоретическое объяснение" этого замечательного факта... http://groups.google.com/group/sci.physics/msg/841.. ... Пара ( Io + Callisto ) и пара ( Europa + Ganymede ) захвачены в резонанс масс 1:1, которому Александр Тимофеев скромно и основываясь исключительно на принципах интеллектуальной собственности присвоил свое имя . ...
[ Сохраненная копия ]  Ссылки http://www.scientific.ru/dforum/altern/1140531797 -- 13.6 Кб -- 11.04.2016
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44. http://www.astro.spbu.ru/staff/ilin2/PAPERS/ICAR99/abstract
Dust around Herbig Ae/Be Stars: Porous, Cometary-like Grains? ... This brings up the question, which we try to answer here, of how the grain porosity affects the observational manifestations of the dust shells of HAeBe stars: the excess infrared emission, anomalous extinction in the ultraviolet, and the peculiar behaviour of colour indices and linear polarization during deep brightness minima observed for about 25% of HAeBe stars (UX Ori, WW Vul, etc). ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/staff/ilin2/PAPERS/ICAR99/abstract -- 3.2 Кб -- 19.11.2010
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45. Contemporary variations on optimal mass transfer problems (Spring 2010)
... Целью курса является ввести слушателей в круг основных современных идей и приложений, развивающихся вокруг классической задачи об оптимальном переносе массы, сформулированной более 200 лет назад Г.Монжем. ... I. Введение в задачи оптимального переноса массы. (4-6 часов, Е. Степанов) . Классическая задача Монжа. ... Существование решений задачи Монжа (решение квадратической задачи, решение линейной задачи в одномерном случае, основная идея решения линейной задачи в общем случае). ... Дробные массы. ...
[ Сохраненная копия ]  Ссылки http://www.mccme.ru/ium/s10/mass.html -- 4.3 Кб -- 01.02.2010
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46. Eruption cosmique dans la galaxie M87 | Ciel et Espace
... Recherche dans le site : . Ciel Espace, le magazine qui vous guide toujours plus loin . ... Ciel Espace, nouvelle formule, c'est . des actualit†йs . ... des pages consacr†йes †а la publication de vos photos Mais c'est aussi une vraie communaut†й avec laquelle partager votre passion et nourrir votre curiosit†й. Accueil Eruption cosmique dans la galaxie M87 . ... Ces jets soul†иvent le gaz froid pr†иs du centre de la galaxie et produisent des ondes de choc dans l'atmosph†иre de M87. ...
[ Сохраненная копия ]  Ссылки http://www.cieletespace.fr/node/5736 -- 28.0 Кб -- 09.04.2016
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47. http://site2010.sai.msu.ru/static/doc/BSafonov_site2010.pdf
Twilight observations with MASS/DIMM B. Safonov Sternberg Astronomical Institute Moscow State University Comprehensive Characterization of Astronomical Sites, 2010 B. Safonov (Moscow State University) Twilight observations with MASS/DIMM SITE 2010 1 / 17 Why observe in twilight with MASS/DIMM? ... ASM includes 3 devices sensitive to background: guider, DIMM and MASS. B. Safonov (Moscow State University) Twilight observations with MASS/DIMM SITE 2010 2 / 17 Background in guider. ...
[ Текст ]  Ссылки http://site2010.sai.msu.ru/static/doc/BSafonov_site2010.pdf -- 705.7 Кб -- 18.10.2010
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48. http://www.adass.org/adass/proceedings/adass03/reprints/P10-2.pdf
... Low resolution, slitless spectral images were obtained at the Loiano Observatory in the wavelength window 3300­6420 ° in order to identify in A, extragalactic ob jects targets displaying the most prominent features that characterise the spectrum of bright hot stars, WR and Luminous Blue Variables (LBV), and of nebular regions as well. ... The two bright H ii regions NGC 5455 and NGC 5461 are clearly identified by the H and [O iii] lines. the current observatory's instrumental set­up. ...
[ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/P10-2.pdf -- 216.0 Кб -- 27.08.2004
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49. The mass and the moment of inertia of the Earth
... МАССА И МОМЕНТ ИНЕРЦИИ ЗЕМЛИ . ... Одним из возможных объяснений разности теоретических и измеренных амплитуд нутационных членов может быть упрощенная модель Земли, состоящей из упругой мантии, жидкого внешнего и упругого твердого ядра. ... The mass and the moment of inertia of the Earth . ... The estimation of the mass and the moment of inertia of the Earth with new model of Moho surface and biased inner core has shown that our result is consistent with the common values. ... Мантия . ...
[ Сохраненная копия ]  Ссылки http://lnfm1.sai.msu.ru/~chujkova/Trudi/zharov.htm -- 13.5 Кб -- 05.08.2002
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50. http://www.gao.spb.ru/english/as/j2014/presentations/kudryashova.pdf
... St Petersburg 23, September 2014 1 Motivation · Origin of Martian moons? ... Considered error sources: ­ Phobos a priori ephemerides; ­ Phobos a priori GM value; ­ measurements noise; ­ different strategies; · Methods: ­ real data analysis; ­ simulations. ... St Petersburg 23, September 2014 8 Simulations: sensitivity of the measurements to the a priori GM value Simulations: zero noise+ IMCCE a priori ephemerides +GMPH = 7.16 * 105 m3/sec2. ... St Petersburg 23, September 2014 14 Thank you! ...
[ Текст ]  Ссылки http://www.gao.spb.ru/english/as/j2014/presentations/kudryashova.pdf -- 482.3 Кб -- 28.09.2014
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51. The Formation and Evolution of LMC Rich Star Clusters: NGC 1818
... LMC Project Outline . NGC 1818 Initial Results . ... The Large Magellanic Cloud (LMC) is uniquely suitable for the study of massive star clusters at all stages of evolution. By combining HST observations of these clusters with N-body models we hope to understand the origin and evolution of rich star clusters in our own Galaxy, in the LMC, and beyond. ... We aim to combine our HST observations with N-body models to understand the formation and evolution of globular clusters. ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node27.html -- 15.4 Кб -- 12.06.2006
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52. Home Page
... A rough estimation is that in the United States there is one planetarium per 100,000 population, ranging in size from the Hayden Planetarium's 20-meter dome seating 430 people, to three-meter inflatable portable domes where children sit on the floor. ... Together dblo associates make a huge impact in the architecture, interior design and development arena in London. ... With the holidays around the corner what better way to spoil your family than with your very own private home cinema. ...
[ Сохраненная копия ]  Ссылки http://www.armagh-planetarium.co.uk/ -- 13.2 Кб -- 14.03.2013
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53. КАРТОТЕКА ПУБЛ?КАЦ?Й СП?ВРОБ?ТНИК?В ГАО НАН УКРА?НИ
ПЕРЕЛ?К ПУБЛ?КАЦ?Й СП?ВРОБ?ТНИК?В ГАО . ... 2014 . ... 2015 . ... No.307, Geneva, Switzerland, June 23- 27, 2014 // IAU Symp., ... Asteroids, Comets, Meteors 2014": Proc. of the conf., Helsinki, Finland, 30 June - 4 July, 2014/ Ed. by K. Muinonen et al. 2014 . ... Rousselot P. Korsun P.P. Kulyk I.V. Afanasiev V.L. Sergeev A.V. Velichko S.F. Ivanova О.V. VizieR Online Data Catalog: Cometary activity of comet C/ 2006 S3 (LONEOS) (Rousselot+, 2014) . ...
[ Сохраненная копия ]  Ссылки http://www.mao.kiev.ua/biblio/cards/show_pub_u.php?start=5980 -- 59.4 Кб -- 10.04.2016
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54. magstorm
After some period of quiet Sun the exciting Sun-Earth connections event as the big magnetic storm was observed at January 10-11, 1997 by various satellites and ground-based instruments. Scientist meet this challenge with unprecedented activity and a few data bases was created in relation with solar event/magnetic storm on a few WEB-sites. ... According the Moscow observatory data the sudden storm commencement (SSC) take place at 01:08 Universal Time of January 10, 1997. ...
[ Сохраненная копия ]  Ссылки http://www.izmiran.rssi.ru/~zaitzev/magstorm.html -- 4.8 Кб -- 17.06.2005
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55. Multiwavelength Study of Mira Ceti-Type Variable Stars
... There are preliminary series of photometric and radio spectral observations of the above-mentioned stars, archival data on the light curves of the stars, results of the search for OH and H 2 O maser emission in IRAS point sources that possess the IR parameters similar to Miras. ... The aim is a detailed study of the maser emission variability. ... In 1996-1997, astronomical observations of Mira Ceti-type stars (miras) were carried out in three spectral ranges: optical, infrared, and radio. ...
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/~gmr/miras.html -- 13.9 Кб -- 25.11.2015
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56. Future of the Galaxy
... We consider the astrophysical evolution of the Galaxy over large time scales, from early stages (an age of ~10 8 yrs) to the end of traditional stellar evolution (~10 11 yrs). ... In the model considered, the basic stages of Galactic evolution are as follows. ... Essentially all other basic parameters of the Galaxy vary little. ... The final "stellar epoch" in the life of the Galaxy is completed ~10 13 yrs after its formation, when the evolution of the least massive stars comes to an end. ...
[ Сохраненная копия ]  Ссылки http://www.inasan.rssi.ru/~dwiebe/abstracts/future.html -- 3.7 Кб -- 27.09.2012
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57. http://www.aaa.org/s932/images/09fallclass3.pdf
Class 1 Introduction, Background History of Modern Astronomy The Night Sky, Eclipses and the Seasons Kepler's Laws Newtonian Gravity General Relativity Matter and Light Telescopes Class 2 Solar System Characteristics Formation Exosolar Planets Class 3 Stars The S un Stellar Evolution of Low and High Mass Stars Deaths of Stars Exotic Stars Class 4 Galaxies Galaxy Classification Formation of Galaxies Galactic ... Low mass stars live and die differently than high mass stars. ...
[ Текст ]  Ссылки http://www.aaa.org/s932/images/09fallclass3.pdf -- 1260.6 Кб -- 07.09.2011
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58. S.P.Korolev RSC Energia - LAUNCHERS
Launch Vehicle Energia . ... The two-stage LV Energia of a package design using a parallel arrangement of stages and a backside accommodation of payload, has four strap-on boosters of stage I (boosters A) arranged around stage II (core stage TS). LV is installed on a pre-launch integration adapter (YA) serving to mate mechanical, pneudraulic, and electric connections between LV and the launch pad and the ground support equipment for pre-launch processing. ... Launch mass, t . ... SEA LAUNCH . ...
[ Сохраненная копия ]  Ссылки http://www.energia.ru/english/energia/launchers/vehicle_energia-c.html -- 11.7 Кб -- 02.10.2012
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59. rgsrmfgen
XMM-Newton Science Analysis System . ... rgsrmfgen generates the response matrices. These are required by rgsfluxer for fluxing spectra, but their true value is seen in such sophisticated analysis packages as XSPEC, where a resolution of 3000 to 5000 incident energy bins (parameter rmfbins ) is recommended for good results. ... The default resolution is set high to avoid misleading the unwary, but lowering it to rmfbins =250 is highly recommended when fluxing is the only use intended. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/rgsproc/node23.html -- 4.9 Кб -- 02.07.2008
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60. Description of the RadioAstron project, english version
... The total mass of the scientific payload is about 2500 kg, of which the unfolding parabolic 10-m radio astronomy antenna's mass is about 1500 kg, and scientific package holding the receivers, power supply, synthesizers, control units, frequency standards and data transmission radio system - near 900 kg. ... The jet system is a hydrazine thrusters system: it will be used during the creation of the base system of spacecraft orientation, for unloading of the powered gyros, and for orbit corrections. ...
[ Сохраненная копия ]  Ссылки http://www.asc.rssi.ru/RadioAstron/description/design_eng.htm -- 6.0 Кб -- 10.05.2008
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