... comedi_dio_config -- change input/output properties of channel . ... int comedi_dio_config (comedi_t * device, unsigned int subdevice, unsigned int channel, unsigned int direction); . The function comedi_dio_config() configures individual channels in a digital I/O subdevice to be either input or output, depending on the value of parameter direction. ... Depending on the capabilities of the hardware device, multiple channels may be grouped together to determine direction. ...

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... These objects are predefined JavaScript objects that you access through the mimeTypes array of the navigator or Plugin object: navigator.mimeTypes[ index ] where index is either an integer representing a MIME type supported by the client or a string containing the type of a MimeType object (from the MimeType.type property). ... Property . ... The Plugin object for the plug-in that is configured for the specified MIME type If the MIME type does not have a plug-in configured, enabledPlugin is null. ...

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• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/plugin.htm
• Objects, Methods, and Properties

Stellarium 0.12.3 . ... Classes . ... FileљStructure . ... SatellitesListFilterModel Class Reference . Custom proxy model allowing filtering by satellite group and flag. ... getFilterFlag () const . ... setFilterFlag (const SatFlag &flag) . QStringљ . ... setFilterGroup (const QString &groupId) . ... setSecondaryFilters (const QString &groupId, const SatFlag &flag) . ... Definition at line 27 of file SatellitesListFilterModel.hpp . ... QString SatellitesListFilterModel::filterGroup . ...

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• Stellarium: MeteorMgr Class Reference
• Stellarium: CCD Class Reference
• Stellarium: CommLink Struct Reference

... CentralProcessor 0.11 documentation . ... The Central Processor Manager is the local monitoring and control agent for the Central Processor sub-system. ... At the moment the Central Processor Manager only controls the acquisition phase; that is, it only controls the ingest pipeline. ... In addition to the CP manager specific parameters, any parameters that begin with ice_properties are passed directly to the ICE Communicator during initialisation. ... string . ... Central Processor Manager . ...

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• casacore: casa::HDF5HidProperty Class Reference
• HI Catalogs Galaxy Properties
• Determining Gains and Polarimetric Properties - GPCAL

... B.1 New functionality . ... B.3 Semantic changes from CSS1 . ... CSS2 builds on CSS1 and all valid CSS1 style sheets are valid CSS2 style sheets. The changes between the CSS1 specification (see [CSS1] ) and this specification fall into three groups: new functionality, updated descriptions of CSS1 functionality, and changes to CSS1. ... Several internationalization features, including list numbering styles , support for bidirectional text , and support for language-sensitive quotation marks . ...

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• Property index
• Long description of example illustrating table row height calculations and
• Media types

... GPI Data Pipeline 1.0 documentation . GPI IFS Data Handbook . ... GPI IFS Detector Properties . ... Detector Gain . ... Operable Pixels . ... The GPI IFS detector is a Teledyne HAWAII-2RG, with 2048x2048 logical pixels (2040x2040 of which are photosensitive, the outer 4 pixels being non-light-sensitive reference pixels). ... The non-operable pixels include about 15,000 hot pixels and 2500 cold pixels that are measured and masked out by the data pipeline. ...

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• Determinations of Dust Scattering Properties from Diffuse Galactic Light (DGL)
• Determinations of Dust Scattering Properties from Reflection Nebulae
• Determinations of Dust Scattering Properties from Dark Clouds

A small paper prepared by V.Tishkovets, P.Litvinov, and S.Beletsky (Kharkov Univ., Ukraina) provides the reader with a brief description of the problem, its solution, the developed software and its training (the PDF version of the paper is here ). ... Please, select the PAS subdirectory for the Pascal version of the code, and the FORT subdirectory for the Fortran version. A brief description of files and their purposes is given in our user notes (their PostScript version is here ). ...

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• Polarization properties (transmitted radiation)
• Database of Optical Properties -- Level: subsubpage
• Extinction properties (transmitted radiation)

... 1) Our CAS system will store the catalogues. ... Each catalogue should contain one or more tables. 2) The names of the catalogues should be unique, as well as the the names of tables of the SAME catalogue. ... 4) All the metadata about the CAS system, its tables, catalogues should reside in separate schema (currently "cas_metadata"). 1) The main system table of CAS is the table "catalog_list". ... short info (column "info") . ... 2) The second system table of CAS is the table "table_list". ...

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• Zen: sncat design

dfos = Data Flow Operations System, the common tool set for DFO . ... business rules . This script checks all vnc sessions running on the muc server for the user account. If one or all are missing (e.g. due to a server reboot), they are created with the session ID and properties as configured in $DFO_CONFIG_DIR/config.dfosVNCserver. ... The tool will check for the configured vnc session IDs and exit silently if all is ok. ... ID: see the business rules for predictable vnc IDs . ... VNC . ...

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• filterRaw
• ESO - Thesis Topic: Properties of kinematically decoupled structures in
• Sample Properties

... AstroGrid Registry . ... 2.Admin Home . ... 1.Submit new resource . ... 3.Get/Find New Registries . ... It is hosted by IVOA, read the admin/index.jsp about e-mailing the registry group the link to your Registry. ... Do the second main link on "/admin/index.jsp" "Register with other Registries" for registering your installed registry to a known full registry. ... Finally do the third main link on "/admin/index.jsp" to become a full registry by grabbing all the registry types of a full registry. ...

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• Spectral properties of X-ray loud e/g sources
• Connect to Database
• The statistical properties of HSS BCGs

. Main Page . Related Pages . Classes . Files . Class List . Class Hierarchy . Class Members . Properties of carbonaceous grains. More... #include < dustmodel.h > . List of all members. double . qgra . double . axi . Properties of carbonaceous grains. The documentation for this struct was generated from the following file: . dustmodel.h . Generated on Fri Jul 11 07:32:08 2008 for DUST by 1.5.5

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• DUST: dustmodel.h File Reference
• DUST: silprops.h File Reference
• DUST: dust_nmoded Struct Reference

... While there is practically no detector noise present at energies above , X-ray data below are considerably contaminated by noise events, which become more and more dominant towards the lowest transmitted energies (Fig. ... Investigations of 40 hours of in-orbit calibration data with the filter wheel closed, taken over a period of more than two years, showed that the noise properties vary with position and energy, but are fairly stable in time for most areas on the detector. ...

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• Description

TH getINDI 1 .SH NAME getINDI \- get INDI property values .SH SYNOPSIS \fBgetINDI [options] [device.property.element ...]\fP .SH DESCRIPTION .na .nh .PP getINDI connects to an indiserver and reports the current value of one or more properties. ... PP The last component of the property specification is usually the element name, but may be a reserved name to indicate an attribute of the property as a whole. ... TP -p <p> connect using alternate port p; the default is 7624. ...

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• http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.1/xmccd-4.1e/indiutil/setINDI.1

... Physical Properties of Crystals . ... The course is an introduction into crystal physics and consists of two introductory parts devoted to the basics of crystallography and tensor analysis and six main chapters in which the physical phenomena in anisotropic medium are described by the example of the elastic, electrical and magnetic crystal properties. The effect of symmetry is also discussed. ... Effect of symmetry on crystal properties. ... Effect of symmetry on crystal optical properties. ...

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• LHPP ISSP RAS
• Grants LSR ISSP RAS
• Laboratory for Spectroscopy of Molecular Structures

. Mars is "behind" the sun from the earth's point of view and is therefore not visible in the nighttime sky (i.e. its up in the daytime). Venus it at greatest elongation and appears in the western sky as a bright object for 2-3 hours after sunset .

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• Orbital Properties of the Earth
• Astronomy HyperText Book

... Consequently, it is inappropriate to expand and in ordinary spherical harmonics. The proper expansion expresses both and simultaneously in terms of a particular order of generalized spherical harmonics. ... Generalized spherical harmonics start at , and for each , . ... Generalized spherical harmonics obey a sum rule analogous to a familiar one for ordinary spherical harmonics, but it includes an explicit phase factor which depends on the orientation of the two lines of sight. ...

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• Synthetic Images of the Solar Corona from Octree Representation of 3-D Electron
• An Infrared Camera Reduction/Analysis Package
• Refining the Guide Star Catalog: Plate Evaluations

About us . ... Telescopes . ... Apart from the 6-meter telescope BTA two small telescopes are operative at SAO: the 1-m and 0.6-m telescopes, both manufactured by Carl Zeiss, Jena, are located near the BTA. ... These telescopes are used for adjusting the equipment and techniques of observations used at the BTA. ... The observational time allocation and also a brief description of the equipment of the 1-m telescope, which is used either permanently or mainly on this telescope, are presented below. ...

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... Measurement of thermal properties of a sample to determine its composition: abundance of sorbed and hydrated water, mineralogical characteristics (chemical composition, crystallization etc.) ... The main registration technique, used in DTA instrument, is measurement of the sample temperature and/or power consumed by the instrument heating cell during the heating with the specified rate. ... Main characteristics of a heater . ... M. Gerasimov, Head of Laboratory +7(495)333-11-55, Mgerasim@iki.rssi.ru...

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• PhSRM
• Magnetic Fields
• Space physics cordinate systems

... The formation of the disks of disk galaxies remains poorly understood. ... Many disk galaxies have only the thin disk component, with no bulge or significant thick disk. ... Almost all disk galaxies have an exponential radial surface brightness distribution. The reason for this exponential form is not known; nor is it known when the exponential form is established. ... We would compare low redshift galaxies observed in the I band with galaxies at z =0.5 in the J band and at z =1 in the H band. ...

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• Host galaxy Investigation Tool for gaMma ray bursts And superNova
• GSAOI High Z Supernovae Science Page

... More than 300 surface reconstructions are already known for pure Si surface and Si surface with adsorbate. Study of their properties by the methods of surface physics reveal numerous interesting phenomena including various phase transitions accompanied by changes of Fermi-surface topology, development of the charge-density wave, etc . ... The charge-density wave (CDW) develops in materials with a chain-like crystal structure at temperatures below the Peierls transition temperature. ...

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• Fractal properties of speech signals - ICND-96
• Research Activities of InformChaos Lab.