... The axial support is provided by 78 air pistons. ... The transverse support is provided by 38 air pistons, supported by cantilevers from the mirror cell, that act on the mirror local center of gravity surface. ... The locations where the transverse mirror support forces should be applied to the mirror are listed in Table 1 and illustrated in Figure 1. ... Figure 1: CAD drawing showing the 2.5-m primary mirror and the locations of the transverse support posts (black) and axial pneumatic pistons (blue...

... Next: Cheating Poisson: A Up: Statistical Analysis Previous: Spatial Models and . ... The spatial distribution of stars in the Local Group dwarf irregular galaxy NGC 6822 has been studied, using recent positions and deep photometry for about 15,000 stars in the galaxy. Based on photometrical data, OB stars and red stars could be studied separately. Spatial statistical tools have been applied to the analysis of the spatial structure. ... Figure: Model selection by the aid of CAIC . ...

... Мировой Центр Данных . ... Мировая система данных МЦД в России и Украине English . ... Данные . ... в Мировой Центр Данных по солнечно-земной физике в Москве ! МЦД по СЗФ является регулярным членом Мировой системы данных Международного совета по науке. ... Наш сайт содержит информацию о МЦД по СЗФ в Москве, его архивах и базах данных, о данных в прямом доступе и о возможности поиска данных, об участии центра в научных проектах и программах, а также ссылки на другие сайты с геофизическими данными. ...

This page is a mirror of the ION SADS page available at http://sads.cnes.fr:8010 . Besides the information already available on this page, there you can browse the ION QuickLook images. ... The ION experiment flown on the Interball-Aurora mission performs simultaneous ion and electron measurements. Two mass spectrometers looking in opposing directions perpendicular to the satellite spin axis, which points toward the sun, measure ions in the mass and energy ranges 1-32 amu and ~ 0 to 14,000 eV. ...

. [ Go back to Comet WWW site ] . Andrew A. Martis . martis @ sai.msu.ru .

... Samara State Aerospace University Staff Timchenko Pavel Evgenevich . ... Raman spectroscopy. ... Timchenko E.V. , Timchenko P.E. , Taskina L.A. and others. ... Timchenko P.E. , Timchenko E.V. , Zherdeva L. A. and others. ... Timchenko E.V. , Timchenko P.E. , Shamina L.A. , Zherdeva L.A. Raman spectroscopy for the control of the atmospheric bioindicators // Remote Sensing and Modeling of Ecosystems for Sustainability XII, 11 - 12 August 2015, San Diego; United States, Publisher: SPIE, 2015, P. 1-8 . ...

... In Fig. 2 the spectrum of the host galaxy HS1035+4758 is shown, in which typical HII-galaxy narrow emission lines are seen: H 4861, [OIII] 4959,5007, H 6562, [NII] 6548,6584 and [SII] 6716,6731 ?. ... The spectral evolution of SN 1998bv is illustrated in Fig. ... The change of the spectrum between April 6 and 19 with clear reddening shortward of H during these 2 weeks indicates seemingly that the 1st spectrum was observed in the period between the 20th and 30th days after the peak of the light curve...

. The SiO (2-1) spectra of N6334 I(N) displayed below (off-source position plus 7-point mosaic) have been obtained in July, 2001, with the one baseline (CA03-CA04: 30m, 2 polarisations) 3mm prototype system of the Australia Telescope Compact Array . The SiO (2-1) rest frequency is 86.847 GHz. Uncalibrated SiO (2-1) emission spectra of N6334 I(N). Fields are: off-source (top left), W, NW, SW, center, NE, SE, E (bottom right). 15-07-2001 * B?rbel Koribalski

We present the results of our observations of the white-light corona in polarized light performed at Criciuma eclipse, Brazil. During the observation of 3.11.94 we have made five couple of pictures of the solar corona in polarization light. ... Koutchmy S., Molodensky M., Starkova L., Ershov A., Matsuura O .: ... Molodensky M., Starkova L., Koutchmy S., Ershov A .: ... Koutchmy S., Molodensky M.M., Starkova L.I . ... Koutchmy S., Molodensky M.M., Starkova L.I. Koutvitsky V. and Ershov A . ...

... Institutes of Chernogolovka . The largest of all the scientific institutions of the center is the Institute of Chemical Physics in Chernogolovka , where fundamental problems of chemical physics are studied: kinetics and mechanisms of chemical and biological processes; processes of combustion, explosion, and polymerization; and mechanisms of elementary reactions involving high energy particles. ... Developments and Technologies . ...

... Here we discuss our survey methods, identification procedure and first results. Our survey is found to be efficient at finding flat-spectrum radio-loud quasars (FSRQs, 59 of our first 85 IDs) and BL Lacertae objects (22 of our first 85 IDs), a figure which is comparable to or greater than that achieved by other radio and X-ray survey techniques. ... Particularly important is the identification of a large population of FSRQs ( of DXRBS FSRQs) with ratios of X-ray to radio luminosity . ... FSRQs . ...

... Address: Space Research Institute (IKI), 84/32 Profsoyuznaya St, Moscow. The Exhibition Participants IKI ­ Space Research Institute , Russian academy of sciences AMI ­ Apply Math Institute , Russian academy of sciences IRE - Institute of Radio-engineering and Electronics of RAS LIPh - Lebedev Institute of Physics, RAS ASC ­ Astro- Space Center , Lebedev Institute of Physics INAS ­ Institute of Astronomy, RAS IAA - Institute of Applied Astronomy ...

... Home Observing Charles Dana Discovery Center, Central Park . ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . ... A History of the First Forty Years of the Amateur Astronomers Association . ... Charles Dana Discovery Center . ... 6:30тАУ8:00 p.m. The Charles Dana Discovery Center is just inside Central Park, near 110th Street between Lenox and Fifth avenues ( map ). ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...

... We apply an additional restrictions on the model which follow from recent helioseismic results: 1) calibration of the surface helium abundance and the specific entropy in the convection zone (Vorontsov et al. ... AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA...

... Department Number . ... Astro Space Center . ... Telephone Number . 7(495) 333 3366 . FAX Number . 7(495) 333 2378 . ... amalin@lukash.asc.rssi.ru . ...

... I.Almar (Konkoly Observatory, Budapest, Hungary), I.Fieges (Satellite Geodetic Observatory, Budapest, Hungary). ... CA), K.Cullers (NASA Ames Research Center, CA), C.Sleeper (Calif. ... The Berkeley SETI Programm: Recent Results from SERENDIP III and the Design and Status of the Next Generation SERENDIP IV System. ... META SETI in Argentina. ... L.Doyel (NASA Ames Recearch Center, Monffett Field, CA, USA). ... E.Prado (NASA Ames Research Center, Monffett field, CA, USA). ...

... Academics . Research Innovation . ... University Psychological Counseling . ... Center for International Education . ... Research Institutions . Research Institute of Astronomy . Research Institute of Biology . Research Institute of Chemistry . ... About the Department . ... The Research Institute of Chemistry (established in 1929) is the first research institute founded at Kharkiv University. ... Chemistry. ... Research Affairs Record Manager of the Research Institute of Chemistry . ...

Wave propagation in an irregular plasma . Methods of the ionospheric plasma radio sounding . ... Program, Grant No. ... Investigation of Anomalous Attenuation Effect Caused by Radio Wave Scattering and Transformation on the Ionospheric Irregularities . ... Grant No. ... Diagnostics of Ionospheric Irregularity Spectrum Using Measurements of Radio Wave Anomalous Attenuation Under Vertical Sounding . ... Simple numerical model of radio wave multiple scattering effects in the ionospheric plasma layer. ...

... In a solar prominence, charged particles stream up from the Sun, spiraling around magnetic field structures poking out of the solar surface, and ultimately fall back along those structures into the Sun. ... As evolution would predict, animals' eyes sense the colors of light emitted most strongly by the Sun. ... The tiny Moon can completely cover the disk of the Sun, blocking most of the emitted visible light, and reveal the Sun's faint outer atmosphere called the corona...a mass of incandescent gas ...

The Youth Space Center of Bauman Moscow State Technical University conducts the workshop for space enthusiasts (only students) every year to provide participants with an opportunity to discuss the results of the year passed in space focusing on Russian and International programs, see and touch the real space hardware and meet people working on the front edge of space science and technology. ... You will go to Mission Control Center and see how the International Space Station is controlled. ...