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http://www.naic.edu/~phil/mbeam/anacom231-2.5.pdf.

1. The Parkes 21cm Multibeam Receiver
The Parkes 21cm Multibeam Receiver is a new facility available on the Parkes Telescope which is operated by the Australia Telescope National Facility (ATNF), CSIRO. The facility consists of a 13-beam cooled 21cm receiver system, located at the prime focus of the 64m dish. ... Completed 21cm Multibeam Receiver being hoisted up to the Parkes focus cabin. ... It is now available, in 64 MHz mode and in pulsar mode, for normal National Facility use. ... Beam 1 . Beams 2-7 . ... Frequency Range . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/multibeam/instrument/description.html -- 8.2 Кб -- 03.02.2013
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2. Available Receivers
... The properties of the currently available receivers are given in Table 3 . The columns of the table give the receiver name, frequency range, the typical System Temperature (T ), Gain, System Equivalent Flux Density (SEFD) and Half Power Beamwidth (HPBW) for zenith angles below 15 (as measured by Arecibo staff.) ... Full details of the ALFA observing system, its performance, how to join an ALFA Consortium, and the latest ALFA news is to be found via, http://www.naic.edu/alfa/ . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~astro/guide/node4.html -- 5.4 Кб -- 22.02.2012
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3. Spectracom 8170 and Netclock/2 WWVB Receivers
... Reference ID: WWVB . Driver ID: WWVB-SPEC . ... This driver supports the Spectracom Model 8170 and Netclock/2 WWVB Synchronized Clock. ... The DIPswitches on this clock should be set to 24-hour display, AUTO DST off, time zone 0 (UTC), data format 0 or 2 (see below) and baud rate 9600. If this clock is to used as the source for the IRIG Audio Decoder (refclock_irig.c in this distribution), set the DIPswitches for AM IRIG output and IRIG format 1 (IRIG B with signature control). ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/~er/xntp/driver4.html -- 5.5 Кб -- 21.12.2007
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4. mod_reqtimeout - Apache HTTP Server
... Apache HTTP Server Version 2.4 . ... Set timeout and minimum data rate for receiving requests . ... Allow 10 seconds to receive the request including the headers and 30 seconds for receiving the request body: RequestReadTimeout header=10 body=30 . ... If the client sends data, increase the timeout by 1 second for every 1000 bytes received, with no upper limit for the timeout (except for the limit given indirectly by LimitRequestBody ): RequestReadTimeout body=10,MinRate=1000 . ... mod_reqtimeout . ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/manual/de/mod/mod_reqtimeout.html -- 12.0 Кб -- 19.11.2015
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5. Monitoring of variable sources at 15 GHz
The Ryle Telescope was used for some years for monitoring variable sources (in addition to its role in source-surveys related to the Sunyaev-Zeldovitch studies). The instrument is now transformed into the "AMI large array": see the AMI pages for details. ... The rebuild took place between 2006 June and mid-2008; between these dates there is no useful data available. ... For some sources there are many plots, organised by date: . ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~guy/ -- 3.6 Кб -- 24.02.2015
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6. List of currently available KP AZ.
Orbital data : INTERBALL AZ GSE and GSM cartesian coordinates, GSE cartesian velocity (once per 10 minutes). ... Magnetic field data from IMAP experiment. Magnetic fileld absolute value and magnetic field index (the difference between absolute value and model value), status flag. ... Counts of H+ and O+ ions are accumulated during one spin period by detectors D6 (antisunward looking), D8 (spin plane), D10 (sunward looking) of TRICS2 subsystem (1.0-30 keV). ... TRICS1, TRICS2, TRICS3 subsystems: . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/ibelova/az_key.htm -- 14.8 Кб -- 12.05.1999
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7. Description of the RadioAstron project, english version
... 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...
[ Сохраненная копия ]  Ссылки http://www.asc.rssi.ru/RadioAstron/description/observations_eng.htm -- 9.5 Кб -- 10.05.2008
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8. mod_logio - Apache HTTP Server
Modules | Directives | ... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Modules . ... Logging of input and output bytes per request . ... Module Identifier: . logio_module . ... This module provides the logging of input and output number of bytes received/sent per request. ... This module requires mod_log_config . This module provides no directives. Custom Log Formats . ... Apache Log Files . This modules adds two new logging directives. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/tb/manual/en/mod/mod_logio.html -- 6.1 Кб -- 10.12.2010
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9. HDF-S Flanking Fields Data Reduction / Technical Issues
... The analysis and reduction of the STIS flanking fields proceeded in similar fashion as for the imaging of the Main STIS Field. ... The DARK calibration reference file used in the CALSTIS data reduction steps was constructed using a 'delta-dark' image appropriate for the epoch of the flanking field observations. ... DRIZZLE drop-size used for the flanking fields was a "pixfrac" of 0.8. ... For information on the data reduction, please read first the technical information for the Main WFPC2 Field . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/science/hdfsouth/reduc_flanking.html -- 9.4 Кб -- 24.05.2000
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10. Description
... Meta Index / Home Page xcolorcod will produce a three-color coded image based on the position and energy of a set of events. ... Assume that in the color table 1 keV corresponds to the color (r,g,b)=(255,128,0). After adding all events the first pixel gets color (255,128,0) and the second (510,256,0). ... Now the first pixel has color (128,64,0) and the second (255,128,0). ... Some more examples using the following color table: 1 keV: (255,128,0) . 8 keV: (0,50,100): . ... 255 128 0 . ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/5.4.1/doc/xcolorcod/node3.html -- 5.6 Кб -- 10.01.2003
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11. Equipment for digital communications
... The set of equipment includes 8-mm band transmitting/receiving module (TRM), 1.5-cm band multi-channel receiver, and 2-cm band receiving module. TRM, operating in 8-mm range, assures two-way communication with up to 10 Mbaud rate (33–36 GHz input/output frequency). The 1.5-cm receiver is designed for receiving the service and scientific data from the space radio interferometer in 18–26 GHz frequency range (8 channels) with up to 36 Mbaud data transfer rate. ... 1.5-cm multi-channel receiver . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/innov/eng/acs30.htm -- 3.7 Кб -- 02.10.2006
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/innov/eng/acs30.htm -- 3.7 Кб -- 02.10.2006
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12. SAI OCL Catalog Description
... Description . Catalog . ... In the Catalog, we publish equatorial (ЮБ 2000 , ЮД 2000 ) and galactic (l,b) coordinates of cluster centers derived as the position of overdensity in 2MASS catalog (Koposov et al. ... Distances, color-excesses and ages are the mean-square values calculated using all available evaluations from different color-magnitude diagrams. ... There are individual pages for every cluster where all available plots and parameters are published. ... 2002). ...
[ Сохраненная копия ]  Ссылки http://ocl.sai.msu.ru/description/ -- 5.9 Кб -- 09.04.2016
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13. Journal "Peremennye Zvezdy"
Peremennye Zvezdy", . ... 11, N 9 (2011) . ... Min . ... min . Comm. 1 . ... MinII = 18.60. ... A very close pair of a faint variable and a brighter neighbouring star (USNO-B1.0 1272-0434523). ... During observations of a poorly studied cataclysmic variable RX J1951.7+3716 (Zubareva Antipin 2011), we discovered four new eclipsing variable stars in close vicinity of the variable. ... To search for new variable stars, we used C-Munipack and VaST (Sokolovsky Lebedev 2005) software. ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/varstars/msg/1250114 -- 13.3 Кб -- 20.10.1971
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14. Description of different types of shell
. There are several different shells available for Unix; the most popular are described here. You can use any one of these shells if they are available on your system. And you can switch between the different shells once you have found out if they are available. Bourne shell (sh) . C shell (csh) . TC shell (tcsh) . Korn shell (ksh) . Bourne Again SHell (bash) .
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/UNIXhelp/shell/oview2.html -- 2.2 Кб -- 17.01.1997
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15. clMonitor
dfos = Data Flow Operations System, the common tool set for DFO . ... dfos tools . ... clMonitor.html, exported to http://qcweb.hq.eso.org/CLUSTER/monitor . ... The clMonitor gives an overview of the currently condor activity (nodes executing condor jobs) and the pending queue. ... idle | ... busy' indicates that condor currently executes a job on that node; 'idle' means no current condor job; 'reserved/not available' means the node is not configured for condor jobs, or is currently not available. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~qc/dfos/clMonitor.html -- 24.2 Кб -- 26.09.2011
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16. Stellarium: TuiNodeFloat Class Reference
Stellarium 0.12.3 . ... Classes . ... TuiNodeFloat Class Reference . Allows navigation but also editing of a float value. ... TuiNodeFloat (const QString &text, QObject *receiver, const char *method, float defValue, float min, float max, float inc, TuiNode *parent=NULL, TuiNode *prev=NULL) . Create a TuiNodeFloat node. ... virtual TuiNodeResponse љ . ... TuiNode (const QString &text, TuiNode *parent=NULL, TuiNode *prev=NULL) . ... virtual TuiNode *љ . ... the default value for the node . ...
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/classTuiNodeFloat.html -- 20.5 Кб -- 28.02.2014
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17. http://crydee.sai.msu.ru/ftproot/pub/comp/os/os2/hobbes/incoming/xwlan312.txt
Upload Information Template for Hobbes.nmsu.edu =============================================== Archive Filename: xwlan312.zip Short Description: Wireless LAN Monitor XCenter Widget Long Description: This XCenter widget allows to monitor the status of your wireless LAN devices, providing connection profile support, automatic connection scan on startup, key generation, WEP and WPA/WPA2 encryption. Available as XCenter Widget and standalone program, Wireless LAN hardware & driver req. ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/ftproot/pub/comp/os/os2/hobbes/incoming/xwlan312.txt -- 2.6 Кб -- 12.02.2016
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18. The Supervisor receiving one of many handouts
... Gallery . ... The Supervisor receiving one of many handoutтАж . Sidebar Left . Sidebar Top . No Sidebar . Sidebar Bottom . Sidebar Right . ... Title: The Supervisor receiving one of many handouts . Description: Image: Kim Rawlings . ... The Supervisor receiving one of many handouts Image: Kim Rawlings . Powered by Gallery 3.0.9 (Chartres) . ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/gallery3/index.php/first100years/album26/IMGP4666 -- 21.5 Кб -- 10.04.2016
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19. Description of database
GENERAL DESCRIPTION OF DATABASE . It is a matter of common knoledge, that solar magnetic fields and, in particular, magnetic fields of sunspots, play important role in many solar events. In Pulkovo observatory the long-term data set of daily observations of magnetic fields of solar sunspots was accumulated, which contains great potential for further researches in solar physics. ... Second section includes files containing sum data about magnetic fields for every observational day. ...
[ Сохраненная копия ]  Ссылки http://www.gao.spb.ru/database/mfbase.old/baseinfo.htm -- 5.7 Кб -- 21.05.2007
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20. Instrumentation
Beginning from the May of the 1997 we started to publish our daily solar radio observations at RATAN-600 radiotelescope. ... Periscope System: South Sector+Flat Mirror . ... It is possible to track a source by moving the secondary mirror along the arc-shaped railway tracks or to perform azimuthal 2D map synthesis . ... 1) It is possible to simultaneously carry out independent observing programs using individual sectors at various discrete azimuths and secondary mirrors on corresponding railway tracks. ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/sun/complex.htm -- 30.8 Кб -- 24.02.2010
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/sun/complex.htm -- 30.8 Кб -- 24.02.2010
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/sun/complex.htm -- 30.8 Кб -- 24.02.2010
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