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1. Arecibo Observatory: S-Low Band Receiver
... S-Low Receiver . ... back to top] . ... Here is a recommended internal memo on this subject : Main Beam and First Sidelobe Parameters for Arecibo's Receiver Systems by C. Heiles et al (5MB PS file ) . ... Receiver History: Used regularly by wide-band pulsar observers. ... Technical Info: To find out the technical details about this receiver, just click on the appropriate icon at the top of the Receiver tabel (Only internally available -- please contact the POC for anything specific). [back to top] ....
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~astro/RXstatus/Slow/slow.shtml -- 12.0 Кб -- 03.02.2013
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2. The Canadian S2 Correlator - Principles of Radio Interferometry
Radio Interferometry Principles . Radio Interferometry Signal Processing . ... A radio interferometer consists of a pair of directional antennas that are tuned to receive radio emissions from a source in a desired RF band. ... The antennas are pointed at the radio source of interest and are set up to receive the signal and process it into a form suitable for transmission to the correlator. ... In connected element interferometry, the digital signal goes directly to the correlator. ...
[ Сохраненная копия ]  Ссылки http://www.gao.spb.ru/english/as/ac_vlbi/principles.htm -- 8.9 Кб -- 26.02.2008
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3. http://www.cplire.ru/html/lab234/pubs/2008_11.pdf
... Special procedures had been developed and tested with the flight electronics: · fast definition of the operational conditions for the FFO (both in the Fiske step and quasi-particle regimes); · measurements of the free-running FFO linewidth; · optimization of the LSU and HM parameters; · optimization of the PLL operation; · minimization of the SIR noise temperature; · setting all predefined SIR parameters in the exact sequence for ... SIS IF dependence on HM voltage and LSU power. ...
[ Текст ]  Ссылки http://www.cplire.ru/html/lab234/pubs/2008_11.pdf -- 490.8 Кб -- 19.01.2009
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4. RadioAstron Monthly Notices
... a) assembling and tuning of printing-circuit boards for the Test-set device and assembling of the Test-set device itself; . ... Engineering models of the On-board Rubidium Frequency Standard (ORFS-SRT) and Space Radio Telescope On-board Heterodyne and Clock Frequencies Synthesizer set (OHCFS-SRT) were packed and delivered to LA to be assembled with the SRT in the Device Container. ... FC                  Focal Container – hermetic package with the scientific payload; it contains receivers, . ...
[ Сохраненная копия ]  Ссылки http://www.asc.rssi.ru/RadioAstron/archives/2003/month_notic/may.html -- 22.7 Кб -- 03.11.2011
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5. INTERNATIONAL SPACE STATION
... Ham packet radio system including: . ... control computer RSC 2. dedicated software monitoring generation of probing pulses in onboard transceiver in radio beacon mode; . ground receiving network of ham radio packet communication to record probing pulses of onboard radio beacon; . ... Generation of onboard radio beacon probing pulses as time marks to ground receiving network (including ham radio receivers of USW) and transmission of the measurement results throughout Internet network. ...
[ Сохраненная копия ]  Ссылки http://www.energia.ru/eng/iss/researches/geophis-12.html -- 9.7 Кб -- 02.10.2012
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6. Generic Reference Driver
... The timecode of these receivers is sampled via a STREAMS module in the kernel (The STREAMS module has been designed for use with SUN Systems under SunOS 4.1.x. It can be linked directly into the kernel or loaded via the loadable driver mechanism). ... The reference clock support in xntp contains the necessary configuration tables for those receivers. In addition to supporting up to 32 different clock types and 4 devices, the generation a a PPS signal is also provided as an configuration option. ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/~er/xntp/driver8.html -- 9.2 Кб -- 21.12.2007
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7. DIGITAL WDC EXCHANGE FORMAT FOR OBSERVATORY 1.0 MINUTE VALUES
DIGITAL WDC EXCHANGE FORMAT . FOR OBSERVATORY 1.0 MINUTE VALUES 1. ... DATA-1 .. DATA-60 are 1-minute values of the given element for that hour. ... Typically, digital 1-minute values received by WDCs from organizations operating automatic magnetic observatory instruments are averages of more frequendy sampled values, e.g. 10-second point samples. ... If the method used to obtain 1-minute average values is important to a user, the WDC will assist in determining the exact procedure applied. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/magbase/HTML/WDCFORM.HTM -- 6.6 Кб -- 03.07.2001
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8. VLBI Wiki | Main / ParkesNotes
... VLBI Schedule . ... Observers Wiki . ... Other VLBI . ... Go to new wiki . ... Main / . Use the official Parkes vnc sessions on joffrey:1 and joffrey:2. Run cdisko and DAS in joffrey:2. ... ssh vlbi@pkvsi1 then das1 . ... 21cm/1.4 GHz . ... where SETUP is the name of the correct session setup file, e.g 2011Mar_HOHa.cmd). ... This file should be copied to Epping and put in the vlbi ftp area /pub/people/vlbi/cal/parkes/logs with the name MonthYear , using a 3 letter abbreviation for the month. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/vlbi/wiki/index.php?n=Main.ParkesNotes -- 17.7 Кб -- 12.04.2016
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9. http://www.stsci.edu/documents/dhb/web/c29_wfpc2data.fm3.html
... Because of the need to schedule observations as efficiently as possible, the order in which exposures are executed may be different from the order in which they appear in the observer's Phase II submission-unless an explicit special requirement dictates otherwise. ... Data files can then be associated with the corresponding exposure line in the Phase II proposal by comparing exposure information in the Phase II proposal with data file header keywords. ... Time_Per_Exposure . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/documents/dhb/web/c29_wfpc2data.fm3.html -- 8.4 Кб -- 17.11.1997
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10. RAS ISR' Conclusion on the scientific results received in the orbital complex
... Director of the RAS ISR . RAS Academician . ... Astrophysics module Kvant of the orbital complex Mir launched in 1987 contains the largest on the station complex of the scientific equipment named the orbital observatory Roentgen. Observatory Roentgen consists of 4 X-ray telescopes, jointly exceeding the range of energies from 2 to 800 keV. ... Among the most significant results that were received in the observatory Roentgen are: . ... measurement of the periods of 9 X-ray pulsars; . ...
[ Сохраненная копия ]  Ссылки http://www.cosmoworld.ru/mirstation/english/documents/iki_ran_280998.shtml -- 11.0 Кб -- 09.04.2016