Журнал ПОВЕРХНОСТЬ публикует оригинальные статьи и обзоры по наиболее актуальным проблемам изучения поверхностных явлений. ... Редакция журнала 'Поверхность. ... Англоязычная версия журнала Journal of Surface Investigation . X-Ray, Synchrotron and Neutron Techniques выходит 6 раз в год . The Journal of Surface Investigation. X-ray, Synchrotron and Neutron Techniques ( Poverkhnost '. ... X-ray, Synchrotron and Neutron Techniques is abstracted and/or indexed in (Impact Factor 0.359): . ...

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

... 2008 August 17 . Io's Surface: Under Construction . Credit: Galileo Project , JPL , NASA . ... Io's surface is constantly under construction . This moon of Jupiter holds the distinction of being the Solar System's most volcanically active body -- its bizarre looking surface continuously formed and reformed by lava flows. ... The notable absence of impact craters suggests that the entire surface is covered with new volcanic deposits much more rapidly than craters are created. ...

... Io's Surface: Under Construction . ... 21.03.1997 . ... Io's surface is constantly under construction . This moon of Jupiter holds the distinction of being the Solar System's most volcanically active body -- its bizarre looking surface continuously formed and reformed by lava flows. Generated using 1996 data from NASA's Galileo spacecraft, this highest resolution composite image of Io is centered on the side of Io that always faces away from Jupiter. ... Publications with keywords: Io . ...

Next: Particle Background Rejection Up: Detection Efficiency Previous: Front Illumination . ... The method requires that the CCD substrate be etched from the rear towards the depletion layer boundary. The device can be illuminated through this rear surface, which has a much thinner dead layer than the electrode side. ... The corresponding detection efficiency data are presented in Figure 7, and compared with the predicted data for a 20 m thick depletion layer. ...

. These pages will highlight work on the road resurfacing project at Apache Point. There will be pages added as work progresses. Enjoy. 20040406: Preliminary markings . 20040416: Cut and cleared asphalt . 20040420: Cut and fill, cut and fill . 20040421: Work, work, work, work, work . 20040423: Surface pullouts and seams . 20040426: Surface upper drive . 20040427: Surface lower drive . 20040429: Almost there

Ice Volcanoes Reshape Europa's Chaotic Surface . Ice-spewing volcanoes and the grinding and tearing of tectonic plates have reshaped the chaotic surface of Jupiter's frozen moon Europa, images from NASA's Galileo spacecraft reveal. ... Although the images do not show currently active ice volcanoes or geysers, they do reveal flows of material on the surface that probably originated from them, said Galileo imaging team member Dr. Ronald Greeley of Arizona State University, Tempe. ... Europa . ...

... The forcing by the solar wind is able to modify this field, creating a cavity called the magnetosphere. ... The outer boundary of the magnetosphere is called the magnetopause . In front of the dayside magnetopause another boundary called the bow shock is formed because the solar wind is supersonic. ... Solar wind and the magnetic field it carries along ( IMF ) modify the form of the magnetosphere, by pushing it in in the dayside and creating a long magnetotail in the nightside. ...

... A closed surface (i.e. a compact surface without boundary) is homeomorphic to either a sphere with g handles (a connected sum of a sphere with g tori) or to a sphere with g M obius bands attached (a connected sum of a sphere with g copies of RP 2 ). A compact surface with boundary is homeomorphic to a closed surface with a nite number of disks deleted. ... Prove that on the sphere with g handles the maximal number of nonintersecting closed curves not dividing this surface is equal to g. IV.11. ...

Next: Tapes Up: Using Disks and Other Previous: Floppies . A CD-ROM drive uses an optically read, plastic coated disk. ... CD-ROM drives are slow compared to hard disks. ... The slowness means that CD-ROM drives are not as pleasant to use instead of hard disks (some Linux distributions provide `live' filesystems on CD-ROM's, making it unnecessary to copy the files to the hard disk, making installation easier and saving a lot of hard disk space), although it is still possible. ...

Selected (two) topical problems in solar / stellar modelling Stellar Astrophysics Centre Improving solar physics by studying other stars GЭnter Houdek The effect of the surface layers on the oscillation frequencies Asteroseismic ages and heavy-element abundances of the Sun solar-like stars Courtesy of J. Christensen-Dalsgaard IAU-GA-SP13 ­ Beijing ­ August 2012 Observed solar frequencies m-averaged frequencies from MDI instrument on SOHO Observed ...

... Kirby, E., Jerjen, H., Ryder, S., Driver, S., Deep Near-IR Surface Photometry of 57 Galaxies in the Local Sphere of Influence , AJ, 136, 1866 (2008) . Kirby, E., Jerjen, H., Ryder, S., Driver, S., 2007, to appear in proceedings of "Galaxies in the Local Volume", Sydney, July 2007 (astro-ph/ 0709.2192 ) Deepest Near-IR Surface Photometry of Galaxies in the Local Sphere of Influence . Kirby, E., Jerjen, H., Ryder, S., Driver, S., The Maximum Baryonic Content of a Galaxy , in preparation . ...

The main reflector surface was measured and then adjusted in jan01. ... cband cals measured jan01 using sky and absorber ) . ... The cband frequencies used were 4500, 4860, 5000, and 5400 Mhz. 8 sources were tracked (although only 2 or 3 were complete tracks) and the gain, SEFD, and pointing errors were computed. ... When the cband cals were measured in jan01 there was a discrepancy in the cal values computed using the absorber or the sky for frequencies greater than 5000 Mhz. ...

... 2009: Europa Lander: Science Goals and Experiments Introduction Europa's complex surface is the consequence of physical processes in the ice shell and in the deep interior. ... Tidal deformation induces pressure changes and therefore may drive currents in the ocean. ... This allows for the determination of the ice shell thickness. cold brittle ice thin ice layer completely frozen ocean Europa's Response to Tidal Forcing h 2 Elastic response of the ice shell. ...

... Ciel Espace, le magazine qui vous guide toujours plus loin . ... 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 La photo la plus pr†йcise de la surface du Soleil . ... Dans des conditions optimales, le t†йlescope devrait parvenir †а une r†йsolution de 45 km †а la surface du Soleil. ... 28/01/2016 - La c†‡te Est des Etats-Unis comme neige au Soleil . ...

... Astrophysics Group . ... COAST . COAST Astronomical Results . Surface Imaging of Betelgeuse . ... Betelgeuse is a nearby red supergiant star, about 500 times larger than the Sun. ... Each image was taken through a different colour filter. From left to right, the images show how Betelgeuse appears in red (a wavelength of 700 nanometres), very near-infrared (905 nm), and near-infrared (1290 nm) light. To show this, we have coloured the images different shades of orange and red. 700 nm . ...

In this method the fields outside and inside a particle are represented by expansions in term of proper basis functions (practically always the vector spherical harmonics). Since the particle surface does not coincide with the coordinate surface, it is impossible to satisfy the boundary conditions exactly, and the expansions are limited by a finite number of terms, and the boundary conditions are considered in a finite set of points (matching points). ...

... V.V.Shevchenko, Sternberg State Astronomical Institute, Moscow University, Universitetsky 13, Moscow 119899, Russia, shev@sai.msu.ru . ... 1.Sternberg State Astronomical Institute, 119899, Moscow, Russia. shev@sai.msu.ru . ... V.V.Shevchenko, Sternberg State Astronomical Institute, Moscow University, Moscow 119992, Russia, shev@sai.msu.ru . ... 119992 Moscow, Russia; . ... 2Sternberg Astronomical Institute, Moscow University, Moscow, 119992, Russia, . ... Moscow, 119992, Russia shev@sai.msu.ru . ...

ATM Forum Message . ... Post . ... Testing Convex Surfaces. ... Post Message | ... There are several ways to test convex surfaces. You can test through the glass. ... Next is making a test plate and doing the convex measurement just like doing two flats against each otehr. ... Next is using a larger lens to test the surface. ... www.astronomy.net . ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

... Информация Руководство и преподаватели Ивлиев Николай Александрович . ... Публикации . ... Колпаков В. А. , Ивлиев Н.А. Атомно-молекулярная модель граничного трения в микротрибоконтактах поверхностей полупроводниковых и диэлектрических материалов // Журнал технической физики. ... Ивлиев Н.А. , Колпаков В. А. ИЗМЕРЕНИЕ ЧИСТОТЫ ПОВЕРХНОСТИ ПОДЛОЖЕК МЕТОДОМ ТРИБОМЕТРИИ // ПРИБОРЫ И ТЕХНИКА ЭКСПЕРИМЕНТА. ... Колпаков В.А. , Ивлиев Н.А. , Колпаков А.И и др. ... 846) 335-18-26 Факс: (846) 335-18-36 . ...