... comedi_dio_read -- read single bit from digital channel . ... int comedi_dio_read (comedi_t * device, unsigned int subdevice, unsigned int channel, unsigned int * bit); . The function reads the channel channel belonging to the subdevice subdevice of device device. The data value that is read is stored in the location pointed to by bit. This function is equivalent to comedi_data_read(device,subdevice,channel,0,0,bit). ... Return values and errors are the same as comedi_data_read(). ...

Stellarium 0.12.3 . ... ClassљList . ... StelLocationMgr Class Reference . Manage the list of available location. ... locationForString (const QString &s, bool *ok=NULL) const . ... Get whether a location can be permanently added to the list of user locations The main constraint is that the small string must be unique. bool StelLocationMgr::deleteUserLocation . ... Return the StelLocation for a given string Can match location name, or coordinates. bool StelLocationMgr::saveUserLocation . ...

... CentralProcessor 0.11 documentation . ... The following parameters determine where the measurement sets are that hold the data to be processed. The default behaviour is to read the MS from the given Scheduling Block (SB) directory. ... Location (on galaxy) of the scheduling blocks. This is used when specifying SB numbers - the default is the standard location for BETA operation. ... These parameters determine which beams in the data to process. ... User Parameters - Pipeline & job control . ...

... Dust :: EBins . ... References dust_EBins::Emax , dust_EBins::Emin , dust_EBins::n , and dust_EBins::Teqi . ... References AllocatePointers() , dust_EBins::Emax , dust_EBins::Emin , dust_EBins::n , and dust_EBins::Teqi . ... References dust_EBins::Emax , dust_EBins::Emin , and dust_EBins::Teqi . ... References DeletePointers() , dust_EBins::Emax , dust_EBins::Emin , dust_EBins::n , and dust_EBins::Teqi . ... References dust_EBins::Emax , and dust_EBins::Emin . ... References dust_EBins::Teqi . ...

... Apache HTTP Server Version 2.4 . Apache > HTTP Server > Documentation > Version 2.4 > Modules . ... Location /server-info> SetHandler server-info </Location> . You may wish to use mod_authz_host inside the <Location> directive to limit access to your server configuration information: <Location /server-info> SetHandler server-info Require host example.com </Location> . ... For example, http://your.host.example.com/server-info?config will show all configuration directives. ?<module-name> . ...

... This file contains a single extension, BADPIX , describing the locations and several characteristics of the pn CCD bad pixels. These are pixels which exhibit a signal in a high proportion of readout frames and/or anomalously high signals. ... Keywords to describe the contents of the CCF: . ... Code of the bad pixel table (BPT) version described in the CCF. ... Type of the bad pixel listed. A bad CCD pixel can be: . ... hot : a pixel that contains a signal almost at every readout of the CCD. ...

... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Modules . ... To enable mod_dav , add the following to a container in your httpd.conf file: . ... In addition, a location for the DAV lock database must be specified in the global section of your httpd.conf file using the DavLockDB directive: . ... In order for mod_dav to manage files, it must be able to write to the directories and files under its control using the User and Group under which Apache is running. ...

Design and Construction of the GHRS . ... The locations of important elements are shown. Figure 6.2: - The focal plane of HST and the definitions of the V2, V3, U2, and U3 axes in the coordinate system of the spacecraft. Figure 6.3: - Locations of GHRS apertures relative to spacecraft axes. Note that the sense of the x and y motions are shown by the arrows, but that the zero point for each aperture (LSA and SSA) is located at its center. ... Figure 6.4: - Optical Schematic of the GHRS. ...

... Co-ordinate systems description . Directories structure . The file names' construction . The file set description . ... The orbital information for each month is presented in the separate directory. The INTERBALL orbital data are located on the STDA server, for each month in the separate subdirectory, which name consists from the year (YYYY) and month (MM) numbers. The Parent Directory of the Tail Probe orbital data is http://www.iki.rssi.ru/da/interball/tail/orbit/ . ...

... They are concerned with Attitude Control System of the spacecraft, satellite visibility from tracking stations, limits on the satellite autonomous operations during the orbit, and needs for auxiliary operations with the spacecraft. ... Among the operational constraints the most important one is the number of programmed slews per orbit, which determines the maximum number of radio sources to be observed during one orbit. ... System temperature (K) . ... Progress of the RadioAstron Project in Pictures...

... When are new sefd curves made . ... The fit types used . ... When the new sefd curve is installed it contains two dates: . The starting date for this sefd curve. ... yyyy ddd This is the start of a sefd curve set of data. yyyy ddd is the start date for the sefd curve. yyyy is a 4 digit year (2004) and ddd is the day number of the year counting from 1. all other lines are sefd curve data. ... azterms1 : c4*cos(az) +c5*sin(az) + c6*cos(2az) + c7*sin(2az) + c8*cos(3az) +c9*sin(3az) . ...

Multichannel Flare Spectrograph . ... phi - the angle between the green vertical line passing through the solar disk image and the violet radius vector "r" of the object located at the center of the spectrograph slit- red cross. positive - clockwise, negative - counterclockwise . ... mx = x coordinate of the coelostat main mirror . ... x : carthesian solar coordinate alog axis parallel to solar equator (in arcsec) . y : carthesian solar coordinate alog axis parallel to solar axis (in arcsec) ...

... Documentation for the Python objects defined by the project is divided into separate pages for each package, module, and class. The API documentation also includes two pages containing information about the project as a whole: a trees page, and an index page. ... A description of the package. ... A summary of the classes defined by the package. ... The module contents frame contains a list of every submodule, class, type, exception, function, and variable defined by a module or package. ...

... Denmark: ftp://ftp.dmi.min.dk/pub/Data/WDCC1/indices/kp-ap/ . Germany: ftp://ftp.gfz-potsdam.de/pub/home/obs/kp-ap/ . ... we do not guarantee the correctness of the international sunspot number R; these values are published separately (Brussels, Belgium) The following scientific and format documentation is adapted from ftp://ftp.ngdc.noaa.gov/STP/GEOMAGNETIC_DATA/INDICES/KP_AP/kp_ap.fmt The subscript p means planetary and designates a global magnetic activity index. ...

dfos = Data Flow Operations System, the common tool set for DFO . ... download: . reference.installation from www.eso.org/~qc/dfos/tools if DFOS . ... The tool is called once from the command line and creates the web page dfosExplorer.html under $DFO_MON_DIR. ... The tool scans all DFOS tools against a reference installation (see below), checks their version, provides links to update if a mismatch is found, links to the documentation pages, and offers editing of the associated configuration files. ...

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. ...

... This is possible at modest cost due to the low moments of inertia of the telescope and enclosure. ... This same performance will be achieved in higher winds when the telescope enclosure is facing away from the wind, or by using wind screens. ... The telescope system (MILT) will be remotely operable with an on-site operator's assistance by an astronomer located at one of the ARC member institutions. ... Mean Wind Speed . ... Offsets > 10 deg: 1 arc sec rms max . ... 5 sec max, tracking to tracking . ...

. In an effort to provide a centralized database for indexing locations and descriptions of Shuttle debris, the editors of Astronomy Net have generated a database and web page where reports can be logged. This may or may not prove useful for cataloging debris reports, but Astronomy Net is happy to dedicate computer resources to help out any way possible. We express our sympathy and prayers to the families and friends of the Columbia crew. If you have located Shuttle debris, report it here.

... Main . ... Telescope . ... Diameter of the main mirror, mm . ... The length of the telescope tube, mm . ... Weight of the main mirror, kg . ... Weight of the main mirror in holder, kg . ... Weight of the telescope, kg . ... field of . ... 1:7.7, with corrector . ... 1:7.7, without corrector . ...

... Tonight's Sky . ... The Magazine . ... Star Atlas . ... An artificial comet holds secrets to Earths life . ... Astronomy for Kids . ... Observing springtime deep-sky objects with a large telescope . ... The planet has extreme temperature swings and perhaps active lava flows. ... A digital supplement to Astronomy magazine. ... Join TravelQuest International with Astronomy and Discover magazines on one of three great tour options surrounding this celestial spectacle . ... Astronomy Magazine . ...