... 2007 November 7 . The Sloan Great Wall: Largest Known Structure? ... Explanation: What is the largest structure known? ... A grouping of galaxies known as the Sloan Great Wall was discovered in the Sloan Digital Sky Survey and is a leading candidate. The Sloan Great Wall can be seen in this digitally recast contour map of galaxies in the Two Degree Field galaxy survey. ... The labeled Sloan Great Wall spans over one billion light years, longer than any structure ever measured. ... About APOD | ...

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• APOD: November 6, 1997 - The Magnetic Carpet Of The Sun
• APOD: November 20, 1997 - Escape From The Sun
• APOD: 2003 November 10 - An Intermediate Polar Binary System

... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...

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... Development of Ideas of Structure and Evolution of Stars. Integral Features of Stars, Which Determine Their Structure, Direction and Rate of Evolutuion. ... Connection between Potential and Thermal Energy of Star. ... Structure of a Main Sequence Star. Features of Massive Stars Evolution on the Main Sequence. Internal Structure of the Sun. ... White Dwarfs, Their Features. ... Evolution from the Main Sequence of Massive Stars. ... Evolution of Small Mass Stars till White Dwarfs Sequence. ...

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• Solar Physics
• Solar-Terrestrial Connections

I'm interested in the structure of interstellar ``clouds'' (filaments, sheets, or whatever) of gas and dust over a wide range of scales, from Galactic spiral arms to AU-scale features -- also how these structures form and interact. ... The possibility of clumpy dust scattering in the Pleiades reflection nebula, which might explain its otherwise surprising UV scattering properties . ... Intricate structure of H I emission and self-absorption in the CGPS . ... Fractal studies of molecular clouds . ...

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• Galactic Spiral Structure in H I Emission and Self-Absorption
• First Galfa H I Map

... 172 ] Briefly, the count rate at the detector from a source at a redshift z is . ... Figure 55 shows the ``Green functions'' for the double compact binary merging rate   evolution assuming no collapse anisotropy. ... Another way that diverse peculiarities in the - distribution induced by the sources evolution could arise is connected with a possible non-monotonic character of the star formation rate in galaxies. ... 22 ] Figure  56 shows two-dimensional cuts through the parameter space. ...

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• Evolution of Magnetic Rotators in Non-circular Orbits

... An ionospheric trough is a region of decreased F layer plasma density. ... It is quite typical to make a distinction between the sub-auroral troughs at mid-latitudes, and high-latitude troughs within the auroral region or polar cap . ... working for mid-latitude trough and some types of high-latitude troughs, like the polar hole . ... Collis, P. N., and I. HДggstrЖm, Plasma convection and auroral precipitation processes associated with the main ionospheric trough at high latitudes, J. atmos. terr. ...

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• International Conference "MODE CONVERSION, COHERENT STRUCTURES AND TURBULENCE"
• Substorm fine structure [Oulu]
• Plasma waves [Oulu]

... In addition, Aladin can now parse VOTables from various origins. ... Compatibility with VO standards The emerging VO standards are already implemented in Aladin, allowing users to access VO image and data servers, immediatly available in Aladin by describing these servers in the GLU registry. ... VOTable VOTable has been the first IVOA standard. ... It allows to access various servers of astronomical catalogues, as well as metadata descriptions such as SIA and IDHA servers (see below) 2.2. ...

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• CFITSIO, v2.0: A New Full-Featured Data Interface
• Design and Implementation of CIA, the ISOCAM Interactive Analysis System
• ADASS 2003 Conference Proceedings

... November 30, 1999 . Henize 70: A SuperBubble In The LMC . ... Explanation: Massive stars -- upwards of tens of times the mass of the Sun - profoundly affect their galactic environment. ... It is actually a luminous "superbubble" of interstellar gas about 300 light-years in diameter, blown by winds from hot, massive stars and supernova explosions , its interior filled with tenuous hot expanding gas. ... About APOD > . ...

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• APOD: November 8, 1996 - A Solar Corona Ejection
• APOD: 2000 November 8 - October Skylights
• APOD: November 5, 1997 - The Milky Way's Gamma-Ray Halo

... Magnetic fields, subatomic particles, etc., traveling in different directions fill the universe. Do they deflect or otherwise affect one another? If so, isnт??t the information we get from them distorted? ... Neutrino astronomy, which is still in its infancy, is attractive because neutrinos interact so weakly with matter that few of these distorting effects occur. Get instant access to subscriber content on Astronomy.com! ...

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• November 2011 | Astronomy.com
• Astronomy Magazine - Interactive Star Charts, Planets, Meteors, Comets,
• November 2003 | Astronomy.com

... New APT ETC Features and Improvements . for ETC version delivered on November 25, 2003) . ... News and . ... HST Overview . Overview . ... For point sources, the ETC also gives an estimate of the "optimal S/N" (i.e. PSF-fitting method). A new thermal model has been implemented. The Backgrounds and extinction laws have been homogenized with those used by the ETCs of other HST instruments. ... Further information can be obtained from the help link connected to the APT ETC user interface. ...

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• HST this week: 306
• HST this week: 323
• Dust Emission Features in NGC 7023 between 0.35 and 2.5 Microns: Extended Red

... 2 April 1999 . The Nobeyama Radioheliograph data show that in the microwave range, besides large-scale trans-equatorial chains (see, e.g., the May 11-15, 1993 and November 1-4, 1993 events), there are also many examples displaying large and strongly evolving "longitudinal" or "internal" chains connecting remote active regions inside an active zone in one (northern or southern) hemisphere (the August 20-September 3, 1998 event). ... Last update: 2 April 1999 . ...

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• Oct-Nov 2003
• Large_Scale Emitting Chains
• November 4, 2001

... LL Ori and the Orion Nebula . ... This esthetic close-up of cosmic clouds and stellar winds features LL Orionis, interacting with the Orion Nebula flow. Adrift in Orion's stellar nursery and still in its formative years, variable star LL Orionis produces a wind more energetic than the wind from our own middle-aged Sun. ... Also known as M42, the nebula's glowing gas surrounds hot young stars at the edge of an immense interstellar molecular cloud only 1,500 light-years away. ... A roll cloud. ...

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• Tornado and Rainbow Over Kansas

... Observatory . ... Science . ... Science Users Information > Science and Technical Meetings > Conferences 2013 > Deconstructing Galaxies . ... Science Users Information . Observing Facilities . ... Observing with ESO Telescopes . ... Observing Tools and Services . ... Data Handling and Products . ... Science Data Products Forum . ... ESO Data . ... The study of the structure and morphology of galaxies is one of the major tools astronomers have to address how galaxies form and evolve. ...

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• ESO - My data shows an extended, bright feature - what can this be?
• Titan Observed Through Nine Different Filters on November 26, 2002 | ESO
• ESO - Research Area: STELLAR STRUCTURE AND EVOLUTION

Next: Functionality Up: RGS_EXAFS Previous: RGS_EXAFS Contents . EXAFS means Extended X-ray Absorption Fine Structure. This CCF describes the detailed absorption lengths of different layers of CCDs in the vicinity of absoption edges to facilitate accurate calculation of quantum efficiencies. Away from the edges, the well-known Henke coefficients are used. There are two notable RGS instrumental absorption features by oxygen and fluorine. ... Michael Smith 2011-09-20 ...

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• Description
• Extended-source detection Algorithm
• CAL_getRGAObscure

... This is a preliminary summary of the event on November 24, 1996, considered during the INTERBALL Workshop in Kiljavanranta, Finland, February 1998. ... Pronounced plasma sheet thinning (Bz decrease) . ... Particle burst observed inside the Polar Cap and in tail lobes . A short burst of particles detected by the Auroral Probe particle detectors during the Polar Cap crossing at 21:45 UT, almost simultaneously with the Tail Probe detectors registration of the particle burst inside the North Lobe. ...

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• Scientific Programme
• MAGION-4 Spacecraft (C2-X)
• The Earth's Magnetosphere

... Table data are arranged in columns and rows, and stored in MIDAS files with the extension .tbl . ... An item in a table is accessed by giving its column and row in addition to the table name. The row number can either be given as an absolute value (i.e. the sequence number) or indicated by the value in a previously defined reference column. ... A table can be always expanded in the sense that its number of columns and rows is automatically increased when the allocated space is exceeded. ...

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• Local Keywords
• Power of test statistics
• Site Specific Features

... The evolution of magnetic fields in OB-type stars from the study of open clusters of different ages . ... Wade G. A. The MiMeS Project: Magnetism in Massive Stars . ... Polosukhina N., Shavrina T., Drake N., Kudryavtsev D. Smirnova M. New results of the spectral observations of CPstars in the Li I 6708? spectral region with BTA telescope of SAO RAS . ... Magnetic Stars-2010 . ... List of participants . List of reports . ... Laboratory for the Stellar Magnetism Study of SAO of the RAS . ...

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• Fabry-Perot Interferometer: Gallery Old
• LWN: Using read-copy-update
• Dynamic Memory Allocation and Dynamic Structures

... Evolution of the magnetic field (solid lines) , temperature (colour) , and velocity (arrows) at four times for case A1 (a), A2 (b), B1 (c), and B2 (d). The characteristic parameters of magnetic field strength and electron number density are given above each case plot. ... Aims We aim at investigating the formation of jet-like features in the lower solar atmosphere, e.g. chromosphere and transition region, as a result of magnetic reconnection. ...

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• Leonid Press Release
• Taurid Complex
• Bright Point Studies

Stellarium 0.12.3 . ... Classes . ... Scripting . ... Scripting Engine . ... Script Console . ... Since version 0.10.1, Stellarium includes a scripting feature based on the Qt Scripting Engine . ... Prior to version 0.10.0, Stellarium used a different scripting engine called StratoScript . ... Prior to version 0.10.0, Stellarium had a simple scripting engine, known as StratoScript . ... This script prints "Hello Universe" in the Script Console output window. core.debug( "Hello Universe" ); . ...

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• Stellarium: StelShortcutMgr Class Reference
• Stellarium:
• Stellarium: StelMainScriptAPIProxy Class Reference

... Dale A. Gardner . NASA Astronaut (deceased) . ... NASA EXPERIENCE: б  Gardner was selected as an Astronaut Candidate by NASA in January 1978, reporting to the Johnson Space Center in July 1978.б  In August 1979, he completed a one-year training and evaluation period, making him eligible for assignment as a mission specialist astronaut .б  He subsequently served as the Astronaut Project Manager for the flight software in the shuttle onboard computers leading up to the first ...

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• Astronaut Bio: Shannon Lucid (02/2012)
• Astronaut Bio: J. Hoffman 9/02
• Astronaut Bio: John E. Blaha (05/2008)