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... Three or four lectures on isoperimetric inequalities in infinite groups (October) . ... Nash inequalities are useful tools to estimate the rate of decay of return probabilities in term of the spectral geometry of the space (isospectral profile). ... The isospectral profile can be estimate with purely geometric tools: isoperimetric inequalities and Folner couples. 3) Isoperimetric inequalities. ... The Erchler-Gromov isoperimetric inequality for wreath products is an entropic inequality. ...

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• http://zebu.uoregon.edu/1997/ph410/hw4.html
• Astronomy HyperText Book: Fusion Sequences in Stars

... The variability of the spectrum of the optical component of the IR-source IRAS01005+7910 was discovered for the first time in the BTA spectra [1]. ... The spectral features include absorptions that form in near-photospheric layers, narrow envelope emissions, and emission-absorption profiles that form in photosphere-to-envelope transition layers (the wind). ... Discovery of spectral variation in the optical counterpart of IRAS01005+7910. ... Dashed line - envelope curve of all the SiII 5979 profiles ...

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• Solar system sector, archive 2012

... The plasma region above the ionosphere on such closed magnetic field lines is called the plasmasphere. ... In the first approximation, the plasmasphere lies just inside the ring current and the plasma sheet field lines. ... In addition, plasmasphere is asymmetric, having a clear dusk side bulge (Carpenter, 1970; Chappell et al., 1970; see also Carpenter et al., 1993) that swings westward during high geomagnetic activity (Carpenter, 1970). ... Res., ... 75 , 3837-3847, 1970 . ... 75 , 3848-3861, 1970...

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• Pressure pulses [Oulu]
• Field-aligned potential drops [Oulu]
• Auroral arcs [Oulu]

... R = 97% C8F 18 MO PA /4 P MO PA 160 В 350 ps; up to 0.5 J 90 В 500 ps; up to 0.5 J small SBS -mirror reflectivity small amplifier energy extraction thermal aberrations in Nd:YAG pulse compression up to 150ps energy stability StDev532nm 6.5% SBS -mirror reflectivity 97% Gaussian output beam profile phase-conjugated beam pulse compression up to 90ps energy stability StDev532nm 3% Example of SBS - pulse ...

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• Keywords_52

... Centrifuge . ... Technical description centrifuge TSF-7 . ... If during rotation the operator feels badly, the hand will release, and the centrifuge will stop. ... Tests for cosmonauts: . ... Services / Centrifuge: General description Technical description Photo gallery Price . Info: Industry news On-line Data Company ATLAS news Events We in press Contact . Copyright 2000-2016 ATLAS Aerospace . ...

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... The air just sit there and doesn't get stirred. ... Normally, the air is hottest near the ground and gets cooler as you go up. ... If it weren't for the temperature profile, convection wouldn't occur: Because the temperature decreases with altitude, cold air sits on top of hot air, allowing convection. ... The air above the ground is hot, the air above the water is cold. ... The land cools down faster than the sea, so the air above the ground is colder than the air above the water. ...

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• ASP: Corporate Affiliates
• ASP: Women in Astronomy: An Introductory Resource Guide to Materials in English

COPRATES CHASMA NORTH WALL INTERIOR LAYERED DEPOSIT: LAYER MEASUREMENTS AND COMPARISON WITH JUVENTAE CHASMA ILDS USING MARS EXPRESS HIGH RESOLUTION STEREO CAMERA (HRSC) DERIVED TOPOGRAPHY Michael, G.1, E. Hauber1, K. Gwinner1, R. Stesky2 ... Planets, Freie Universitaet, Berlin, Germany 5ESTEC, ESA, Noordwijk, The Netherlands Introduction: The interior layered deposit ( ILD ) in the north wall of Coprates ... The lesser section of the ILD is confined by a ridge of the chasma wall. ...

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• http://selena.sai.msu.ru/Chik/Publications/Aitken/MS015.pdf
• http://selena.sai.msu.ru/Greg/Publications/ms38/ms067.pdf
• http://selena.sai.msu.ru/Greg/Publications/ms38/ms090.pdf

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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Blackholes2 Forum Message . ... Post . ... Light Pulses . ... Post Message | ... Posted by Herb S. on November 8, 2002 05:11:20 UTC . ... Speed of light - jon0902 - November 17, 2002 - 14:32 UTC . It does not accelerate- it has no mass - yaniru - November 18, 2002 - 01:42 UTC . ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

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• VISTA - Visible and Infrared Survey Telescope for Astronomy

... Line radiative transfer in C 18 O, HCO + , and CS lines is considered in a spherically symmetric chemo-dynamical model of a starless core, evolution of which is driven by the ambipolar diffusion. Theoretical line profiles are compared to observational data on the well-known L1544 core, which is one of possible candidates for collapsing protostellar clouds. ... Comparison between modelled and observed spectra suggests that L1544 has flattened structure and is observed at some inclination. ...

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Some radio clocks and related timekeeping gear have a pulse-per- second (PPS) signal that can be used to discipline the local clock oscillator to a high degree of precision, typically to the order less than 50 us in time and 0.1 PPM in frequency. ... Either way requires conversion of the PPS signal, usually at TTL levels, to RS232 levels, which can be done using a circuit such as described in the Gadget Box PPS Level Converter and CHU Modem page. ...

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• APOD: 2004 April 9 - NGC 4565: Galaxy on the Edge
• APOD: 2005 July 8 - NGC 4565: Galaxy on the Edge
• APOD: 2008 March 8 - M104 Hubble Remix

The low aspect ratio, or spherical tokamak Globus-M [1] has recently been built in a support of international spherical tokamak plasma investigation program. ... The survey to determine the work scope in diagnostic design for Globus-M is given in the paper. ... The next one is an advanced diagnostic set intended to supply the data on basic plasma parameters: electron temperature and density profiles, ion temperature, plasma composition, radiation profile, Zeffective. ... Magnetic Diagnostics. ...

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... The software enables to browse HITRAN-86 or 96 databases. It enables input first 7 atmospheric gases. ... calculate atmospheric transmittance on any pressure level, . calculate instrument transmission functions through the atmosphere, . ... The software is supplied by standard atmospheric profiles, extracted from FASCODE_3.0 FORTRAN codes (dowloaded from PL/GP), and by instrument response function for IR channels of NOAA 14 satellite (both AVHRR and HIRS, downloaded from NOAA/NESDIS). ...

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... Name (for family membership, include all family member names) Address City, State, Zip Code Home Phone Email Address Other Phone Alternate Email Occupation (if retired, list previous occupation; if student, list major) Employer or School My Employer will match my donation Membership List ­ Each year we publish our Membership List with name, city, email and home phone number and distribute this list to all members. ... Student Memberships are for FULL TIME students of any age. ...

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• Amateur Telescope Makers of Boston

... SUN MOON MERCURY VENUS MARS, JUPITER SATURN . Sun . ... The Sun's Heartbeat . ... Can a 0.2-second pulse from a magnetar put out as much energy as the Sun does in 250,000 years? ... A giant magnetar flare is incredibly bright and emits as much radiation energy as the Sun does in hundreds of thousands of years. Get instant access to subscriber content on Astronomy.com! ... Much more! ... If you are already registered on Astronomy.com, please log in below. ...

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• A curious cold layer in the atmosphere of Venus | Astronomy.com
• White dwarf pulses like a pulsar | Astronomy.com

We present a catalogue of galaxies for which spatially resolved data on their internal kinematics have been published; there is no apriori restriction regarding their morphological type. The catalogue lists the references to the articles where the data are published, as well as a coded description of these data: observed emission (E) or absorption (A) data, optical (O) or radio (R) data, velocity (V) or velocity dispersion (D), radial profile (1) or 2D field (2). ...

60. Список нарушителей - Общая Астрономическая Конференция