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1. ESO - Processed Calibration Files for VLT instruments Now Available
... Science . ... Science Users Information > Science Publications > Science Announcements > Processed Calibration Files for VLT instruments Now Available . ... ESO Data . ... ESOReflex data reduction workflows can be used to customize the generation of the processed and co-added calibration frames and to apply them to the science files. A detailed step-by-step guide on how to automatically associate the appropriate calibrations, raw or processed, to the science files of interest is available . ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/sci/publications/announcements/sciann15057.html -- 23.6 Кб -- 10.04.2016
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2. Methods and instruments to measure/monitor major site properties
... The Science Operation Department is composed of Astronomers, Telescope Instruments Operators(TIOs) and Data Handling Administrators(DHAs). ... Astronomers have proposed several methods to quantitatively measure the amount of turbulence above the telescope, which the most common ones is Differential Image Motion Monitor (DIMM). In optical testing, the Hartmann test is the common method to test the quality of optical components. ... Hartmann mask consists of 48 lenses. ...
[ Сохраненная копия ]  Ссылки http://site2010.sai.msu.ru/section/2 -- 9.2 Кб -- 09.04.2016
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3. Execution of Commands
Next: MIDAS Command Language Up: Monitor and Command Previous: Input/Output Redirection in . ... The basic commands are executed inside the MIDAS monitor, which is the program you are interacting with. All other commands are implemented by executing a MIDAS procedure љ which runs one or more programs in a subprocess (child process). During the time a command is being processed in the subprocess, the MIDAS monitor is suspended until the corresponding program terminates in the subprocess. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol1/node39.html -- 6.0 Кб -- 23.02.1996
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4. Errors in Processed TIME-TAG Data from STIS Now Corrected
... HST . Errors in Processed TIME-TAG Data from STIS Now Corrected . ... Data . ... HST Peer Review Process . ... HST Overview . ... The previous ground processing software failed to properly trap these errors. As a result, gaps or jumps in time could occur in processed TIME-TAG data. ... All investigators working with STIS TIME-TAG data should read the more detailed discussion of possible problems, and if they believe that their data may have been affected, retrieve it again from the archive. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/stis/performance/anomalies/timetag_fixes.html -- 19.7 Кб -- 11.04.2016
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5. ``On-the-Fly'' Calibration System for the ISO Data Archive
Next: Distributed Data Systems, Data Mining . ... Previous: The ISO Data Archive . ... At the end of the mission, all available data were processed and ingested into the ISO Data Archive (IDA) 5 specifically designed at the ISO Data Centre in Villafranca del Castillo near Madrid, Spain. ... Besides the population of the initial archive, this Bulk Reprocessing of the ISO data left the so-called ``auxiliary'' data on disk, which would then be used for the future On-the-Fly Calibration System. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass99/P3-29/ -- 12.3 Кб -- 12.10.2000
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6. IKI IPL home page
You can also see this page in Russian with using KOI8 (X Windows) or CP1251 (MS Windows) Cyrillic coding. The Laboratory supports the space TV experiments, mainly in the planetary exploration missions. ... Image Co-registration . ... PHOBOS mission - Martian satellites investigations. Phobos on the Martian limb, the image from Phobos-2 probe from 02/28/89. ... Russian Space Bulletin. ... Last modified at June,26 1997 Alexey Kuzmin: akuzmin@mx.iki.rssi.ru . Back to IKI home page ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/IPL/ -- 4.8 Кб -- 05.08.1997
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7. Monitoring processes
To monitor the state of your processes use the ps command. ps [-option] . Used without options this produces a list of all the processes owned by you and associated with your terminal. Options for this command vary with the type of UNIX system that you are using. ... It may be that you are running more than one terminal session on the system and/or that you have processes which have no controlling terminal associated with them. ... Understanding process information . ...
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/UNIXhelp/shell/jobz4.html -- 2.8 Кб -- 17.01.1997
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8. Astronomy HyperText Book: Stellar Evolution
... 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. ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/textbook/se.html -- 4.8 Кб -- 16.12.1997
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9. The CIMA ALFA Instrument Monitor Window
. The ALFA instrument monitor window is a big window showing all ALFA engineering parameters (with the exception of the ALFA motor). The 'Open motor control window' button opens the ALFA motor control window . You can return to the main CIMA page by clicking here .
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~cima/cima_show_alfamonwin.html -- 2.0 Кб -- 01.03.2012
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10. http://xmm.vilspa.esa.es/sas/8.0.0/doc/omthconv.ps.gz
XMM-Newton Science Analysis System Page: 1 omthconv July 2, 2008 Abstract Converts OM tracking-history data into tracking-star count-rates time series 1 Instruments/Modes Instrument Mode OM TRACKING 2 Use pipeline processing yes interactive analysis yes 3 Description In order to perform accurate tracking throughout an exposure, software onboard the Optical Monitor(OM) selects n (up to 10) guide stars visible within the FOV and monitors their position and counts during the exposure. ...
[ Текст ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/omthconv.ps.gz -- 44.0 Кб -- 02.07.2008
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11. Central Processor Manager CentralProcessor 0.11 documentation
... 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 . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/askapsoft/sdp/docs/current/services/manager/index.html -- 16.3 Кб -- 12.04.2016
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12. SXG Science Data Center
SXG Data Center . ... Data archive . ... The prototype of archiving and data extracting system was realized for MOXE all-sky monitor long-term data archive . ... The data must be organized in the way that will provide the maximum effectiveness for the goals of long term data analysis i.e. long period monitoring of the particular field of the sky. ... DBM2 field Because the data in DBM2 are stored sorted by the fields on the sky it is the simpliest way to specify which part of the sky is necessary. ...
[ Сохраненная копия ]  Ссылки http://hea.iki.rssi.ru/SXG/SDC/level_1/archive.html -- 5.4 Кб -- 18.02.2004
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13. SMIS IKI RAN (Equipmaent)
... Satellite data ] . ... The SCANOR system provides receiving and processing of the Earth-surface pictures made in visible and infra-red bands and transferred by satellites of the NOAA polar orbiter series (in the HRPT mode). ... The SCANOR system includes the desktop receiving device connected to an IBM AT 386 type computer, and the parabolic antenna with the guiding mechanism. The SCANOR system possesses the state-of-art software providing registration and processing of the received data. ...
[ Сохраненная копия ]  Ссылки http://smis.iki.rssi.ru/inform/engl/equip_e.htm -- 6.3 Кб -- 12.01.1999
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14. Rev0, US-Processed Data
Next: Rev0, MPE-Processed Data Up: DETAILED LIST OF ROSAT Previous: DETAILED LIST OF ROSAT . Prior to June 1994 data processed in the U.S. were supplied in the following files: . ... rp<seq#>.fits . Photon events, data quality, and good time intervals (binary table) . ... Compressed image for display -- total energy band . ... Compressed image for display -- hard energy band . ... Compressed image for display -- soft energy band . ... Selected source spectra (ascii table) . ... Aspect files . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node192.html -- 8.3 Кб -- 01.10.2012
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15. MARSES Homepage | Instrument Information
Marses Instrument . ... Currently we use a Tem-fast 48 sounding instrument that is based on time domain electromagnetic sounding technology. ... Areas of application are following: . ... hidrogeological research, . ... Despite many competitors' instruments with similar areas of application, Tem-fast 48 has reasonable advantages among small depth sounding devices. ... The Tem-fast 48 sounding instrument consists of following devices: . ... The block diagram of the sounding instrument is outlined below. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/MARSES/english/instr.htm -- 7.9 Кб -- 03.09.1999
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/MARSES/english/instr.htm -- 7.9 Кб -- 03.09.1999
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16. http://www.arcetri.astro.it/science/irlab/doc/adass_94.ps
Distributed Software for Observations in Near Infrared V. Gavryusev 1 and C. Baffa Osservatorio Astrofisico di Arcetri E. Giani Dipartamento di Astronomia, Universit`a di Firenze Abstract. ... The processes denoted for control of hardware (telescope and other instruments) should be executed currently on PC dedicated for this task under DESQview/X, while all other components (user interface, tools for the data analysis, etc.) can work also under Unix. ... 1993, Di Giacomo et al. 1993). ...
[ Текст ]  Ссылки http://www.arcetri.astro.it/science/irlab/doc/adass_94.ps -- 1609.9 Кб -- 28.07.2005
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17. Actor Prolog. Example "D:\MOROZOV\Z\DEMO\EXE\EXAMPLES\SADT\JAM-E\JAM-E.A"
An example of visual expert system. The program is written on Actor Prolog. -- -- (c) Alexei A. Morozov, March 19, 1999. ... Actually I wrote this program to train myself -- -- in carrying out SADT interview. ... A logical description of the blocks of the SADT model. ... The main purpose of these classes is keeping lists of cooking -- -- battery corresponding to various blocks of the SADT model. ...
[ Сохраненная копия ]  Ссылки http://www.cplire.ru/Lab144/start/e_jam_a.html -- 33.0 Кб -- 24.09.2007
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18. LS 3.5" Color LCD Video Monitor
STEP INTO THE BLUE - MEADE INSTRUMENTS PRODUCT GUIDE . ... Meade 4M Community . ... Meade Instruments . ... Telescopes . LX850 Series . ... Superb optical performance coupled with time proven computerized pointing and tracking has made the LX200 ACF series a best-seller in the high-performance telescope class. ... Coronado Accessories . ... LS 3.5" Color LCD Video Monitor . ... This full color monitor plugs directly into the built in camera on the Meade LS-6 and LS-8 LightSwitch telescopes. ...
[ Сохраненная копия ]  Ссылки http://www.meade.com/ls-3-5-color-lcd-video-monitor.html -- 83.4 Кб -- 09.04.2016
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19. Radioastrophysical department ISTP RAS SB
RADIOASTROPHYSICAL DEPARTMENT  INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . ... Radioastrophysical Department , Institute of Solar-Terrestrial Physics, Siberian Division, Russian Academy of Science. ... Head of Laboratory dr. Gubin A.V. LABORATORY of INFORMATION SUPPLY and METHODOLOGY of RESEARCH . ... Head of Observatory Kitsanov S.V. SIBERIAN SOLAR RADIO TELESCOPE . Siberian solar radio telescope data at 5.7 GHz in I SOHO EIT 171 SOHO EIT 195 SOHO EIT 304 MDI Continuum MDI Magnetogram . ...
[ Сохраненная копия ]  Ссылки http://ssrt.iszf.irk.ru/ -- 20.8 Кб -- 09.04.2016
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20. stecf.impol - Features
Next: stecf.impol - Package Tasks Up: stecf.impol - an IRAF Previous: stecf.impol - an IRAF . All the instrumental set-up, such as filters, polarizers, rotation angles, etc. are read from the image headers. Many input images ( 3 < N < 64) can be processed. ... Output images can be rebinned to increase the polarization signal-to-noise per output pixel. ... Output error images have fully propagated statistical errors from the input error images. ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/adass99/P2-21/node6.html -- 3.7 Кб -- 06.06.2006
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