... This function can also be used for particular types of subtypes or kinds: KIND (0) integer KIND (0.0) floating point number KIND (.FALSE.) logical variable KIND ("A") string of characters There is an intrinsic function SELECTED_REAL_KIND , which returns the kind of the type REAL that has a representation with (at least) the precision and the exponential range requested. ... With the choice SELECTED_INT_KIND (5) all integers between (but not including the limits) -100 000 and +100 000 are permitted. ...

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... First the task demos (``de-mosaic'') is used to break the model produced by mosmem into models for individual pointings. ... Task selfcal takes all the models simultaneously and then, for each visibility in the input visibility dataset, it computes a model visibility using the model with the same pointing centre. ... DEMOS . ... There are, however, multiple input models (produced by demos ) corresponding to each of the pointings to be used in the self-calibration. ... Models produced by demos . ...

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• The Interpolation Process
• Data Selection CentralProcessor 0.11 documentation
• Preventing Gain Interpolation - GPBREAK

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... First three columns show base-difference images of the evolution of the wave in 3 EUV channels (211 , 193 , 171 ) of AIA in which the wave is clearly visible. ... From our study we have quantitatively confirmed previous results that during wave passage the plasma visible in the Atmospheric Imaging Assembly (AIA) 171 channel is getting heated to higher temperatures corresponding to AIA 193 and 211 channels. ...

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• CONCLUSION (2)
• Astrodynamics 101
• BUT :

... In Figures 2-2, 2-3, 2-4 spot diagrams corresponding to the minimum dispersion configuration at zenith, maximum dispersion at 60° and ADC compensation at 60° are shown. ... Date:04.06.98 Page 2 of 6 Figure.2-1 Camera and ADC with curved surfaces in the maximum dispersion configuration Figure.2-2 Spot corresponding to the configuration of minimum dispersion at zenith 2 Document : VST_040698_optic.doc Release :1 First rel.date: 04.06.98 Last rel. ... Date:04.06.98 Page 5 of 6 Figure. ...

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• IBIS - Installation
• Solar Mystery Nears Solution With Data From SOHO Spacecraft
• TRASP 2

... A Colorful Moon . ... But small, measurable color differences have been greatly exaggerated to make this telescopic, multicolored, moonscape captured during the Moon's full phase. ... In most places on Earth, a lucky viewer.. Geminid Meteors over Teide Volcano . ... Gibbous Europa . ... In fact, this gibbous phase shows part of Jupiter's moon Europa. ... The Bubble Nebula . ... Cataloged as NGC 7635, it is also known simply as The Bubble Nebula. ... What will survive this battle of the galaxies? ...

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• Journal "Peremennye Zvezdy"
• The ISS and a Colorful Moon
• A Colorful Moon

... Character codes are given in hexadecimal when available for the Postscript symbol set and HP's math -8 symbol set. ldots; \ldots three dots on the baseline cdots; \cdots three dots on same level as a minus sign vdots; \vdots three vertical dots ddots; \ddots diagonal dots (top left to bottom right) dotfill; \dotfill like cdots but fills column in an array thinsp; \, thin space sp; \: medium space emsp; \; thick ...

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• Modern variants of UNIX
• Entering carriage returns
• More about the UNIX operating system

... Gravity data reflect changes, related to the groundwater redistribution, ice melting, and precipitation accumulation. ... We apply Multichannel Singular Spectrum Analysis (MSSA, or extended EOF) technique to filter GRACE data and separate the principal components (PCs) of different periods. We performed data averaging over the large river basins of Russia. ... Fig 1. ... MSSA is a promising method for GRACE data processing, de-striping, filtering, and Principal Components (PCs) separation. ...

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• IDL programs

.

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• Bishop School: Day and Night
• The AstroStat Slog Blog Archive Where is ciao X ?
• The AstroStat Slog software

... The results of long-term monitoring of Gigahertz-Peaked Spectrum sources were found the statistically significant differences (0.05 significance level) in the high-frequency spectral index distribution between subgroups of galaxies and quasars. ... This can mean that the electron energy distribution for GPS galaxies is steeper than for GPS quasars. ... The first area corresponds to GPS-quasars that have statistically larger value of redfhift, second area corresponds to GPS-galaxies. ...

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• New Polar Ring Galaxies
• Electronic version of Russian Bulletin
• Metagalaxy sector, archive 2000

... Starting from a grid of theoretical population synthesis models we constructed a set of model galaxies with a distribution of ages, metallicities and intrinsic reddening. ... We propose an optimization technique that combines active learning with an instance-based machine learning algorithm. ... In order to solve the problem more efficiently, we pose it as a learning problem, where a learning algorithm learns the reddening parameters , and with a forward model we compute . ... Let be the test set. ...

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• A Computer-Based Technique for Automatic Description and Classification of
• Unified Survey of Fourier Synthesis Methodologies
• The Astrometric Properties of the NOAO Mosaic Imager

... Such particles are called ``optically soft'', and the corresponding approximation could be named that of optically soft particles. ... For the theory based on the assumption (1), there are a set of the names: Rayleigh-Gans [ 11 ], Rayleigh-Debye [ 274 , 397 ], Rayleigh-Gans-Born [ 474 ], Rayleigh-Gans-Debye [ 78 , 144 , 409 , 410 ], Rayleigh-Gans-Rokard [ 132 ], Rayleigh-Debye-Gans (RDG) [ 100 , 462 ], Born (or the first Born) [ 56 , 135 ] approximation. ...

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• Polarization properties (transmitted radiation)
• Circular polarization: change of sign
• Database of Optical Properties -- Level: subpage

Crater Gassendi . ... I made this drawing was made on the 26th of november 2001. If you compare this one with the previous drawing of Gassendi (below) the differences are clear. ... This drawing was made on the 28th of september 2001. After nearly a full month without observations I had a one hour gap between the thicker clouds. ... This drawing was made on the 29th of august 2001. ... This drawing was made on the 27th of august 2001. ... This drawing was made on the 25th of august 2001. ...

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Instructions for using Menu-driven Axis Control Software . ... Altitude and azimuth axes use position feedback and the setting is in counts per second times 10. ... Use b to set the brakes and use c to clear the brakes for the corresponding axis, either azimuth or altitude. ... Use m to move to the previously specified position and velocity for the corresponding axis; either azimuth or altitude. ... Use g to move to the previously specified position and velocity for both the azimuth and altitude axis. ...

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• Tracking error budget
• TUI:Instruments:NICFPS:NICFPS window
• TUI:Instruments:Echelle:Echelle window

. N OTE: . Only clusters with R<60 kpc were used to compute the spatial parameters and metallicity gradients for all subsystems except the corona. The numbers in parantheses give the number of clusters for which the corresponding parameter is known. The X O scale length of the old halo is strongly distorted by the observed asymmetry of the distribution of the corresponding clusters projected onto the XY plane ( Fig. 4А ) . discussion in the text | previous table .

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• Population of Galactic globular clusters, figures
• Doclad, figures
• F-stars in galactic disk, figures

... The image combines data acquired with the PACS instrument at 70 micron (corresponding to the blue channel) and 160 micron (corresponding to the green channel) and with the SPIRE instrument at 250 micron (corresponding to the red channel). ... Credits: ESA/PACS/SPIRE/Martin Hennemann Fr†йd†йrique Motte, Laboratoire AIM Paris-Saclay, CEA/Irfu тАУ CNRS/INSU тАУ Univ. ...

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B2740D5E3-CB4C-46C5-A490-42FB3F9DC92A%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B3E0CFFB6-07D2-428F-BDC0-4837CEF5A043%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B96ECDA74-55EC-444A-B2EC-C78FC970DEDD%7D

THE PARAMETERS INVOLVED IN HAPKE'S MODEL FOR ESTIMATION OF THE COMPOSITION OF THE EJECTA LUNAR TERRAINS. ... In the previous papers we were estimated the surface roughness of the ejecta lunar terrains by means comparison of the local phase function and the average integrated lunar indicatrix. ... The Hapke's theoretical model of the lunar surface reflection. ... For THE PARAMETERS INVOLVED IN HAPKE'S MODEL: S.G. Pugacheva, V.V. Shevchenko a low-albedo lunar surface parameter Bo = 1. ...

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• http://selena.sai.msu.ru/Bus/Publications/LPSC2001a/LPSC2001a.pdf
• http://selena.sai.msu.ru/Bus/Publications/UFN2007(Bus_etal)(engl).PDF

... A comparison of the computed and experimental relations F max ( H), as well as comparison of drift scans of point sources across different horizontal cross-sections of the BP with the corresponding computed cross-sections were made. ... The drift scans of the point source 3С84 (H=87 o ) at the wavelength 7.6 cm across the horizontal cross-sections of the BP (black lines) and the computed horizontal cross-sections of the BP corresponding to them (red lines). ...

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• String Manipulation
• Linux Device Drivers, 2nd Edition: Chapter 10: Judicious Use of Data Types
• Application-specific functions

Stellarium 0.12.3 . ... Classes . ... FileљStructure . ... StelToneReproducer Class Reference . ... Set the eye adaptation luminance for the display (and precompute what can be) Usual luminance range is 1-100 cd/m^2 for a CRT screen. ... Set the eye adaptation luminance for the world (and precompute what can be) More... љ . ... Return adapted luminance from world to display. ... Return adapted luminance from world to display with 1 corresponding to full display white. ... xyYToRGB (float *xyY) const . ...

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... Its apparent diameter of 18.0 arc minutes corresponds to a linear extension of about 180 light years; Kenneth Glyn Jones mentions an estimate of even 20 arc minutes from deep photographic plates, corresponding to about 200 light years linear diameter. It appears somewhat smaller in amateur instruments, perhaps about 10 minutes of arc. ... Red: 20x3 minute subs, totaling 1 hour . Green: 20x3 minute subs, totaling 1 hour . ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

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It is difficult to do experiments with K?12 students which demonstrate that light involves electric and magnetic fields. ... For advanced students, these experiments can show how light reveals the structure of atoms. ... Visible light penetrates glass. ... Static, unchanging magnetic fields don't spawn electric fields, and steady electric fields don't create magnetic fields. ... Light and other forms of electromagnetic radiation contain both electric and magnetic fields that oscillate in strength. ...

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• ASP: Family ASTRO: Race to the Planets
• ASP: Family ASTRO: Night Sky Adventure
• ASP: Black Holes to Blackboards: In the Seventh House of Saturn