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1. Basic training program for a cosmonaut/astronaut or a manned space flight
... Space flight . Crew training . ... The contemporary world opinion, while welcoming the efforts of different states aimed at realization of manned space flights, still considers these efforts insufficient, over-bureaucratized and too slow. ... The more up-to-date is the basic training program for a cosmonaut/astronaut or a manned space flight participant (hereinafter referred to as the student) that is being offered to your interested attention. ... Pre-flight space training (PFST). ...
[ Сохраненная копия ]  Ссылки http://www.atlasaerospace.net/eng/podgotovka.htm -- 33.4 Кб -- 09.04.2016
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2. TrueTime GPS/GOES/OMEGA Receivers
... Reference ID: GPS, OMEGA, GOES . Driver ID: TRUETIME . ... This driver supports several models models of Kinemetrics/TrueTime timing receivers, including 468-DC MK III GOES Synchronized Clock, GPS- DC MK III and GPS/TM-TMD GPS Synchronized Clock, XL-DC (a 151-602-210, reported by the driver as a GPS/TM-TMD), GPS-800 TCU (an 805-957 with the RS232 Talker/Listener module), OM-DC OMEGA Syncrhonized Clock, and very likely others in the same model family that use the same timecode formats. ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/~er/xntp/driver5.html -- 5.5 Кб -- 21.12.2007
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3. 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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4. Arecibo Observatory Narrow S-Band Receiver (2.24-2.42 GHz)
... S-Band Radar (2.24 - 2.42 GHz) . ... Receiver History . Contact Info . ... It is normally left in the higher range, which is the band used by the Arecibo Planetary radar. If you expect to need to adjust it, contact us in advance to make sure that it's working. [back to top] . ... Info . ... To see an up-to-date plot of Tsys, just type tsys on your terminal after logging into Arecibo's computer network. [back to top] . ... The lower filter (2.24-2.34) is not well characterized. [back to top] . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~astro/RXstatus/Sradar/Sradar.shtml -- 12.4 Кб -- 03.02.2013
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5. Venera 15 & 16
... USSR Venus Orbiters . ... Each spacecraft consisted of a synthetic aperture radar (SAR) and a radio altimeter. ... The Venera 15 and 16 synthetic aperture radar (SAR) systems were identical, and were used to map the surface of Venus at a resolution of 1 to 2 kilometers (.6 to 1.2 miles) over a period of 8 months. ... The Venera 15 and 16 radar (radio) altimeter systems were identical, and were used to determine the topography of the surface of Venus from the north pole down to about 30њN latitude. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/Astro/solar/eng/venera16.htm -- 8.8 Кб -- 15.03.1998
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6. 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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7. 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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8. Astronaut Bio: Robert L. Stewart
... Robert L. Stewart (Brigadier General, USA, Ret.) ... SPECIAL HONORS: Awarded Army Distinguished Service Medal , Defense Superior Service Medal , 2 Legion of Merit, 4 Distinguished Flying Crossed, a Bronze Star, a Meritorious Service Medal , 33 Air Medals, the Army Commendation Medal with Oak Leaf Cluster and V Device, 2 Purple Hearts, the National Defense Service Medal , the Armed Forces Expeditionary Recipient of NASA Space Flight Medal (1984 & 1985). ...
[ Сохраненная копия ]  Ссылки http://www.jsc.nasa.gov/Bios/htmlbios/stewart-rl.html -- 8.7 Кб -- 07.07.2015
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9. Description of the RadioAstron project, english version
Status of the RadioAstron project development . The engineering model of the Space Radio Telescope (SRT) was assembled in Lavochkin Association (LA) in the configuration consisting of 10-m parabolic radio astronomical antenna made of carbon-fiber, F ocal and Device cabins of the scientific payload and on-board and ground complex of high data rate up-down radio link (VIRK). ... Then,radio astronomical tests were conducted using real radio sources. ... Space Radio Telescope . ... Data Processing . ...
[ Сохраненная копия ]  Ссылки http://www.asc.rssi.ru/RadioAstron/description/status_eng.htm -- 7.2 Кб -- 10.05.2008
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10. 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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11. Topics in AstroStatistics
Modern AstroStatistics has emerged as a new field in recent times, informed by a Bayesian foundation, utilizing powerful computational tools like MCMC, and applied to diverse analysis and inference problems in Astronomy. ... The goal of our Special Session is to review current practices, highlight modern techniques, and explore how the transition into the realm of Big Data Astronomy can be facilitated. ... Big Computing in Astronomy: Perspectives and Challenges . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/AAS224/ -- 12.5 Кб -- 10.04.2016
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12. Venera 15 & 16
USSR Venus Orbiters . ... Venera 15 and Venera 16 were a two-spacecraft mission designed to use 8-centimeter (3-inch) band, side-looking radar mappers to study the surface properties of Venus . ... Each spacecraft consisted of a synthetic aperture radar (SAR) and a radio altimeter. ... The Venera 15 and 16 synthetic aperture radar (SAR) systems were identical, and were used to map the surface of Venus at a resolution of 1 to 2 kilometers (.6 to 1.2 miles) over a period of 8 months. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/solar/eng/venera16.htm -- 7.6 Кб -- 15.10.1997
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13. Karazin University
... International programs . ... Information Consolidation in International Anti-Crisis Management . ... European Diploma Supplement . ... AљDIPLOMA SUPPLEMENT isљaљdocument given toљgraduates ofљhigher educational institutions ofљall forms ofљproperty and subordination toљprovide information required for objective evaluation ofљhigher education qualification (degree) received byљthe person awarded with aљhigher education diploma. ... Copyright 2010 V.љN. Karazin Kharkiv National University. ...
[ Сохраненная копия ]  Ссылки http://www.univer.kharkov.ua/en/study/euroDiploma -- 18.0 Кб -- 09.04.2016
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14. 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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15. HwB: Macintosh RS-422 Connector
It's possible to connect RS-232 peripheral to the RS-422 port available on Macintosh computers. Use RXD- as RXD, TXD- as TXD, Ground RXD+, Leave TXD+ unconnected, GPi as CD. At the computer) . 8 PIN MINI-DIN FEMALE at the computer. ... TXD- . Transmit Data (-) . ... Receive Data (-) . ... GPi . ... Receive Data (+) Note: Direction is DTE (Computer) relative DCE (Modem). Note: GPi is connected to SCC Data Carrier Detect (or to Receive/Transmit Clock if the VIA1 SYNC signal is high). ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/drabek/Components/NewSprawoch/connect/co_MacRs422.html -- 5.0 Кб -- 26.10.1999
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16. http://star.arm.ac.uk/~jgd/outgoing/Armagh_CU/PDF/Risk_Listing.pdf
Armagh Credit Union Risk Register Policy Number 1 Risk Area SCV Risk Description Lack of updated address Likelihood / Possible Impact / Probability Cost Low Measure Implemented Last Review Date Mar '15 Members unable to Followup AGM returns annually for receive payment if change of address required by the FCA/PRA Loss of member (s), ...
[ Текст ]  Ссылки http://star.arm.ac.uk/~jgd/outgoing/Armagh_CU/PDF/Risk_Listing.pdf -- 77.5 Кб -- 18.12.2015
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17. http://www.stsci.edu/documents/dhb/webvol2/c12_ghrserrors.fm9.html
... The DCF staff perform a check of the transmission using a Reed-Solomon error checking routine. ... Missing data packets and the results of the Reed-Solomon check are written to the data quality accounting capsule (QAC). ... d1h file, there is a corresponding data point in the quality file. For each good data value, the corresponding point in the quality file is zero. ... If the data failed the Reed-Solomon error check, the corresponding data point in the quality file was set to one. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/documents/dhb/webvol2/c12_ghrserrors.fm9.html -- 4.8 Кб -- 10.02.1998
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18. ASP's 2012 Annual Meeting
... Annual Meeting . ... Registration . ... Online registration is now closed. ... Check or money order -- via postal mail accompanied by a printout of the confirmation email you receive after submitting your online registration. ... For the Early Bird or Advance rate your check or money order must be received by the deadine for that rate in order to receive the reduced rate. ... If you are new to the ASP , you are invited to become a member in order to receive the member rate for registration. ...
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/events/2012mtg/registration.html -- 28.1 Кб -- 30.07.2012
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19. Description of SED models
... FTP access the basic models is here . ... Below, we put short descriptions of the used SED models for the photometric redshifts providing by the current server . ... The uniqueness of this model consists in expanding to the near IR (NIR) of Rocca-Volmerange and Guiderdoni's (1988) atlas of synthetic spectra with a revised stellar library, which includes parameters of cool stars. ... Homepage of the GISSEL model). ... Another model used earlier is the model of synthetic spectra of Poggianti (1997). ...
[ Сохраненная копия ]  Ссылки http://sed.sao.ru/sed_E_models.html -- 9.2 Кб -- 12.01.2005
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20. Astrophysics Group VSA
... Astrophysics Group . ... VSA . ... CAT . ... The Very Small Array is a custom-built radio telescope (operating between 26-36 GHz), designed expressly to make high resolution observations of the cosmic microwave background (CMB) radiation on angular scales around and below one degree. ... The VSA has been operated in ?compact array? and ?extended array? configurations (see the technical description below) and data collected to achieve high sensitivity in both regimes have been analysed. ... 1.75 GHz)...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/outreach/radio-telescopes/vsa/ -- 20.2 Кб -- 10.04.2016
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