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21. http://xmm.vilspa.esa.es/sas/8.0.0/doc/omcomb.ps.gz
... Invalid x- image size ( fatal ) f ilename Invalid y- image size ( fatal ) f ilename 4 image les are required ( fatal ) only N were provided Invalid WINDOWXO value (x) for le name ( fatal ) WINDOWX0 should be either 0, 512, 1024 or 1536 2 FILES ( name and name ) have identical WINDOWX0 values ( fatal ) Invalid WINDOWYO value (x) for le name ( fatal ) WINDOWY0 should be 0 ... 4) Check that this WINDOWX0 value is not identical to one of the previous values. ...
[ Текст ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/omcomb.ps.gz -- 45.9 Кб -- 01.07.2008
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22. http://www.ipa.nw.ru/conference/2002/sovet/PS/KESHIN.PS
... 8, ``Celestial Mechanics'', 2002 First results of GPS orbit determination with GRAPE package using a square--root information filter M. O. Keshin Institute of Applied Astronomy, St. Petersburg, Russia The zero--differenced carrier phase measurements contain the distance be­ tween the phase centres of receiver and transmitter antennas biased by unknown integer number of cycles (phase ambiguities). ... In the case of GPS the problem of solar radiation pressure modelling is of primary importance. ...
[ Текст ]  Ссылки http://www.ipa.nw.ru/conference/2002/sovet/PS/KESHIN.PS -- 28.3 Кб -- 19.08.2002
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23. 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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24. 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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25. International Astronomy Olympiad 2010, resolutions
... Resolution to be issued: . For reports, received before June 11: not later than 15 days after receiving . For reports, received on June 12-21: not later June 27 . For reports, received on June 22 - June 27: not later July 27 . For reports, received on June 28 - July 16: during the week July 26-30 . For reports, received on July 17-31: not later 4 weeks after receiving . ... Dr. Michael G. Gavrilov, Founding Chairman and Coordinator of the International Astronomy Olympiad (IAO) . ...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/iao/2010/ia10rt_e.html -- 9.6 Кб -- 30.08.2010
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26. ARC 3.5m | Instrumentation
... ARC 3.5m | Instrument Summary . ... ARCES (Echelle) : the ARC Echelle spectrograph, a high resolution (R~31,500) echelle spectrograph that observes the entire wavelength range from 3200 е to 10000 in a single image on a 2048x2048 CCD. This instrument is permanently mounted at the NA1 port. ... In addition to the facility instruments, several visitor instruments have been used at the 3.5m, and some of these are available to the ARC observing community by contacting the instrument PIs: . ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/arc35m/Instruments/Instrumentation_ARC35m.html -- 7.5 Кб -- 09.10.2014
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27. Hewlett Packard 58503A GPS Receiver
... Driver ID: GPS-HP . ... This driver supports the HP 58503A Time and Frequency Reference Receiver. ... It receiver should be operated with factory default settings. Initial driver operation: expects the receiver to be already locked to GPS, configured and able to output timecode format 2 messages. The driver uses the poll sequence :PTIME:TCODE? to get a response from the receiver. ... Specifies the driver reference identifier, an ASCII string from one to four characters, with default GPS . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/~er/xntp/driver26.html -- 4.2 Кб -- 21.12.2007
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28. http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt_satellites.pdf
To appear in "Fourth Workshop on Robotic Autonomous Observatories (2015)"RevMexAA(SC) MASSIVE PHOTOMETRY OF LOW-ALTITUDE ARTIFICIAL SATELLITES ON MINI-MEGATORTORA S. Karpov, 1, 3 E. Katkova,2 G. Beskin, 1, 3 A. Biryukov3,4 S. Bondar,2 E. Davydov5 E. Ivanov,2 A. Perkov,2 V. Sasyuk3 RESUMEN Favor de prop orcionar un resumen en espanol. ... The nine-channel Mini-MegaTORTORA (MMT-9) optical widefield monitoring system with high temporal resolution system is in operation since June 2014. ...
[ Текст ]  Ссылки http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt_satellites.pdf -- 185.1 Кб -- 15.12.2015
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29. Meade Instruments Corporation - Pictor Manual Index
... Meade Instruments Corporation . ... Meade Pictor XT-Series CCD Autoguider/Imagers . ... Section 1: Getting Started . ... To Take an Image . ... Section 3: File Menu . Section 4: Edit Menu . Section 5: View Menu . Section 6: Image Menu . ... Merge Images . ... Meade Software License Agreement . ... Manufacturer is Meade Instruments Corporation, 6001 Oak Canyon, Irvine, California 92620. ... Index of Instruction Manuals . ... Copyright 2006 Meade Instruments Corporation, All Rights Reserved. ...
[ Сохраненная копия ]  Ссылки http://www.meade.com/manuals/pictor/index.html -- 16.0 Кб -- 10.11.2012
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30. Area of scientific investigations
... Research of an atmosphere of the Earth and other planets of Solar system by optical methods . ... The long-term experience of study of atmospheres of planets of Solar system in a department of physics of planets has defined directions and methods of researches spent for laboratory . ... The tasks of laboratory are researches by optical methods of structure of a Terrestrial atmosphere, namely study of spectra of absorption of its compound radiation of natural and artificial sources. ...
[ Сохраненная копия ]  Ссылки http://www.mao.kiev.ua/lao/investigations_eng.html -- 16.3 Кб -- 12.01.2010
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31. C.J. Butler, Research Astronomer
Next: J.E. Chambers, Research Astronomer Up: Research Previous: Research Contents . ... Solar Variability and Climate . Other Activities . ... Applied to data of flares on Gliese866 he was able to estimate the area of hydrogen emitting flare regions as 1-13% of the stellar surface. ... As partners in the project, Armagh Observatory has been asked to contribute to the selection process in exchange for priority access to the data which will eventually flow from the satellite. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/annrep/annrep99/node10.html -- 10.7 Кб -- 05.05.2000
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32. ApSA courses
Teaching courses . for student of the Department of Astrophysics and Stellar Astronomy . ... Geophysics and physics of the planets (Kurt, Panteleev) . ... Close Binary Stars . ... Solar Physics . ... This is introductory course for students of the third year of education which are familiar with elementary astronomy and general physics. ... The one-year course includes theory of radiation transfer, theory of internal stellar structure with account of binary systems with compact comapnions. ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/asa/ASACours.htm -- 19.5 Кб -- 01.04.1997
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33. INTERCOSMOS 19
... INTERCOSMOS 19 . ... The Intercosmos-19 satellite was designed for investigations of the topside ionosphere structure and electromagnetic processes in it. ... The instruments installed onboard Intercosmos-19 were designed and manufactured by scientists of Bulgaria, Poland, Czechoslovakia and USSR. ... The sounding data could be directly transmitted to a receiving station (direct mode) or be stored in the onboard memory device for a certain period and then sent to the Earth (recording mode). ...
[ Сохраненная копия ]  Ссылки http://www.izmiran.rssi.ru/projects/IK19/ -- 9.4 Кб -- 09.04.2016
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34. Hardware sector, archive 2004
... 2004: . Creation of a unique set of the spectral and polarization complex of high resolution in the range of 6-18 GHz, consisting of 64 channels with a 1% analysis stripe was concluded. Based on the combination of key parameters - the frequency overlap and resolution, sensitivity and accuracy of polarization measurements, such a complex is the first instrument of its kind in the practice of solar astronomy. ... Archive . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/Science/results/ar_facil/res2004.html -- 5.4 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/Doc-en/Science/results/ar_facil/res2004.html -- 5.4 Кб -- 10.04.2016
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35. The Focal Plane Instruments
Next: The Transmission Gratings Up: The Instruments Previous: The Instruments . ... A conventional cross-grid charge detector reads out the photo-induced charge cloud and the electronics determine an arrival time to 16s, and the position with a resolution of about 18 m or 0.37 arcsec. ... The Massachusetts Institute of Technology's Center for Space Research, in collaboration with Lincoln Laboratories, developed the detector system and manufactured the CCDs; Lockheed-Martin integrated the instrument. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~polar/images/chandra/crete_astro-ph/node4.html -- 4.1 Кб -- 07.12.1999
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36. MASTER-II Kislovodsk
M obile A stronomical Sy stem of TE lescope- R obots MASTER-II Kislovodsk Lomonosov Moscow State University, Sternberg Astronomical Institute , Moscow Union "Optic" , Kislovodsk Solar Station Latitude = 43 o љ44'.767љN; Longitude = 42 o љ31'.417љE; Altitude = 2067љm MASTERљIIљ(8љsquareљdegress) + MASTERљVWF(VeryљWideљFieldљCameras (FOV=800 square degrees, Timeљresolutionљupљtoљ150љms, with unfiltered m_lim=14m on 5 sec. exposure, and ~10.5m with 0.15 sec) . ... 11h 38m 38.0s , -09d 59m 59s) . ...
[ Сохраненная копия ]  Ссылки http://apollo.sai.msu.ru/ -- 11.6 Кб -- 09.04.2016
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37. Astronaut Bio: G. Harbaugh 4/01
... GREGORY J. HARBAUGH (MR.) . NASA ASTRONAUT (FORMER) . ... He held engineering and technical management positions in Space Shuttle flight operations, and supported Shuttle flight operations from Mission Control for most of the flights from STS -1 through STS 51-L. He served as Lead Data Processing Systems (DPS) Officer for STS -9 (Spacelab-1) and STS 41-D, Orbit DPS for STS 41-B and STS 41-C, and Ascent/Entry DPS for STS 41-G. Mr. Harbaugh also served as a senior ...
[ Сохраненная копия ]  Ссылки http://www.jsc.nasa.gov/Bios/htmlbios/harbaugh.html -- 8.2 Кб -- 07.07.2015
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38. Young SSAU scientists will guide the orbital constellation of the satellites
... SSAU History . ... The Ground Control Complex for Small Spacecraft of Samara State Aerospace University took control of the satellites Aist-1 . ... The data received from SSAU scientific equipment on board of the satellites Aist-1 was processed by the engineers of the Rocket and Space Centre and then was transferred to the university scientists. ... On April 19, 2013 the first small spacecraft Aist-1 was launched from the space-launch complex Baykonur together with a research satellite Bion-M No. ...
[ Сохраненная копия ]  Ссылки http://www.ssau.ru/engnews/11715/ -- 27.6 Кб -- 24.08.2015
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39. CONICA: The high resolution near-infrared camera for the ESO VLT
... Design of Imaging Optics . Analyzing Optics . ... The high resolution near infrared camera (CONICA) for the first VLT unit telescope is under development. It serves as a multi-mode instrument for the wavelength region between 1.0 and 5.0 microns, providing diffraction-limited spatial resolution when combined with the adaptive optic system NAOS of the VLT (Rosset et al. ... VLT instrumentation, ALADDIN InSb detector, NIR imaging, NIR spectroscopy, re-imaging optics, IR optics . ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node7.html -- 16.6 Кб -- 12.06.2006
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40. http://lnfm1.sai.msu.ru/SETI/koi/articles/abstr2.html
SETI@home consists of a receiving Arecibo antenna, a professional team (PT), and a two-way Internet connection between the PT and an army of S@h users, who load from the S@h server special software for digital signal processing. ... Thereby, METI@home will consist of several originators, which may load via Internet from a M@h server special software for the creation of analog and digital messages. ... Professional Group SETI@home . ... Professional Group METI@home . ... Main Internet Server . ...
[ Сохраненная копия ]  Ссылки http://lnfm1.sai.msu.ru/SETI/koi/articles/abstr2.html -- 6.5 Кб -- 16.10.2002
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