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http://www.iki.rssi.ru/tail/data/ska1/first.html.
http://www.iki.rssi.ru/tail/data/ska1/first.html.
1. How SCA-1 measurements are organized.
The movie demonstrates a succession of 7 complete measurement frames of SCA-1 on rotating Interball-1 spacecraft. Diagram, inspired by Salvador Dali's paintings, shows all 64 viewing directions and 15 energy steps as spheres. ... The distribution of spheres along viewing direction is linear unlike logarithmic distribution in reality. ... Complete 3-D distribution is measured for about 10s. Rotation of the spacecraft during one measurement frame is neglected. ...
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Ссылки http://www.iki.rssi.ru/tail/data/ska1/first.html -- 2.1 Кб -- 11.02.1997
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/tail/data/ska1/first.html -- 2.1 Кб -- 11.02.1997
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[ Сохраненная копия ] Ссылки http://www.cosmos.ru/tail/data/ska1/first.html -- 2.1 Кб -- 11.02.1997
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2. COS Instrument Handbook
COS Instrument Handbook for Cycle 24 . ... Cosmic Origins SpectrographInstrument Handbook for Cycle 24 > Chapter 5: Spectroscopy with COS > 5.9 COS Spectroscopy of Extended Sources . ... COS Spectroscopy of Extended Sources . COS spectra of extended objects can have significantly lower resolution than those of point sources, depending on the spatial distribution of the source. ... A similar situation arises when multiple point sources fall within the aperture. ...
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Ссылки http://www.stsci.edu/hst/cos/design/hst/cos/documents/handbooks/current/ch05.COS_Spectroscopy10.html -- 10.5 Кб -- 12.04.2016
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3. Instrument Orientations and Offset Directions
... IRAF View . This is the orientation of the image as viewed in an image display via IRAF (e.g. ximtool, saoimage). Note: This is different from the orientation of the image as viewed on a Macintosh, via Remark . ... A +X, +Y instrument offset will move a star in the direction indicated by the arrows. ... Note: The offset direction depends upon which interface the offset command was issued in! ... Note: This is different from the orientation of the image as viewed by IRAF. ...
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Ссылки http://www.apo.nmsu.edu/Instruments/offsets.html -- 7.8 Кб -- 06.09.2001
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4. INFRARED FOURIER-SPECTROMETER SICH-F
INFRARED FOURIER-SPECTROMETER SICH-F . ... Instrument work regimes: 1) Inside. 2) Calibration at inside standard sources 2 - 4 times per a rotation. 3) Calibration at "free space" 2 - 4 times per a rotation. 4) Infrared radiation measuring 10 - 40 min. per a rotation. ... Spectrometer consists of the photodetector block and the block of signal processing and control. ... Diagnostic information and attach data will transfer by state telemetric channels. ... Detector temperature. ...
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Ссылки http://space.univ.kiev.ua/projects/warning/sich.html -- 7.5 Кб -- 15.02.2000
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5. http://www.mao.kiev.ua/lao/presentation/grytsai_Ozone%20and%20Strat%20Temp_Kiev%20SSch08.pdf
Variations of total ozone content and lower ozone stratosphere temperature in Antarctic Region during winter-spring period A.V. Grytsai National Taras Shevchenko University of Kyiv Astronomy and Space Physics Department assen@univ.kiev.ua Data, used in the work work Total ozone: Total Ozone Mapping Spectrometer (TOMS) measurements during 1979 - 2005 and Ozone Monitoring Instrument (OMI) ones for 2006, for http://toms.gsfc.nasa.gov/ftpdata.html. ... A long-term TOC decrease is significant. ...
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Ссылки http://www.mao.kiev.ua/lao/presentation/grytsai_Ozone%20and%20Strat%20Temp_Kiev%20SSch08.pdf -- 1659.8 Кб -- 24.09.2008
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6. FM-3I Instrument
Magnetic field measurements onboard the Interball Tail spacecraft are carried out by the FM-3I instrument which consists of two flux-gate magnetometers covering two different ranges: [-200, +200] nT and [-1000, +1000] nT. Besides scientific goals, the FM-3I experiment data is used to perform the attitude control of the Interball Tail spacecraft. ... August 22, 1995 . ... October 18, 1995 . Top of the page . ... Back to the Interball Home Page . ...
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Ссылки http://www.iki.rssi.ru/fm-3i.html -- 2.7 Кб -- 24.05.1996
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7. The AstroStat Slog Blog Archive Redistribution
... Archives . ... It refers to the spread in the measured energy of an incoming photon, and even astronomers often stumble over what it is and what it contains. ... The R edistribution M atrix F ile (RMF) is, at its most basic, a description of how the detector responds to incoming photons. ... The process of measuring the energy introduces a measurement error, which is encoded as the probability that incoming photons at energy E are read out in detector channels i . ... Comment ( RSS ) | ...
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Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2008/redistribution/index.html -- 23.6 Кб -- 01.03.2014
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8. GRANAT Home Page
GRANAT is the Russian x-ray sattelite launched to the high apogee orbit (200,000 km) and operated almost for 10 years (1989 -1999) , carrying out four major instruments: French SIGMA coded-mask hard x-ray telescope (30-1000 keV), Soviet ART-P coded-mask telescope (2??-60?? keV), all-sky monitor WATCH (6-150 keV), and a gamma-burst detector PHEBUS . ... Since September 1994, GRANAT is in the survey mode. ... Explore pages devoted to individual GRANAT instruments (including main scientific results): . ...
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Ссылки http://hea.iki.rssi.ru/GRANAT/granat.html -- 2.5 Кб -- 03.11.2009
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9. The Circinus Galaxy
... Circinus is a nearby spiral galaxy only 4 degrees below the Galactic plane. ... Jones et al. (1996, in prep.) and Koribalski Whiteoak (1996) only recently mapped Circinus with several configurations of the ATCA; a few preliminary results are presented here. ... The elongated central disk (length about 5 arcmin) indicates a bar, and the central `hole' is caused by HI absorption against the bright central region of Circinus. ... Figure 3 : Halpha emission from the nuclear region of the Circinus galaxy...
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Ссылки http://www.atnf.csiro.au/people/Baerbel.Koribalski/circinus/circ_min.html -- 3.9 Кб -- 28.02.2014
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10. A Graphical Planning and Scheduling Toolkit for Astronomical Spacecraft
... A small yet powerful planning and scheduling toolkit has been built for the Submillimeter Wave Astronomy Satellite ( SWAS ) Small Explorer spacecraft. ... The simple design, minimal resource requirements and easy extensibility of the SWAS planning and scheduling toolkit should make it useful for other space astronomy missions. ... The relatively severe time and manpower constraints for the development of the SWAS Planning and Scheduling toolkit have forced it to remain small and simple. ...
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Ссылки http://www.adass.org/adass/proceedings/adass94/kleiners.html -- 11.3 Кб -- 03.11.2000
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11. http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0169-1-1.ps.gz
XMM-Newton CCF Release Note XMM- CCF -REL-169 EPIC MOS low energy response and Quantum Eфciency R. D. Saxton, Steve Sembay 5 August 2004 1 CCF components Name of CCF VALDATE EVALDATE Blocks changed XSCS ag EMOS1 QUANTUMEF 0016. CCF 2000-01-01 QE TOTAL NO EMOS2 QUANTUMEF 0016. CCF 2000-01-01 QE TOTAL NO EMOS1 REDIST 0035. CCF 1999-12-10 2000-07-15 CCD REDISTRIBUTION-n NO EMOS1 ... This excess was responsible for small underestimates of the Galactic absorption column. ...
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Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0169-1-1.ps.gz -- 68.4 Кб -- 10.09.2004
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12. http://selena.sai.msu.ru/Rod/Publications/ms34/MS060.pdf
... The areas between the contours were measured automatically. The results of the measurement are represented on fig.1 The graphic shows the distribution of the height levels against their areas. ... USGS, USA Fig.1 The dependence of the distribution of the heights levels versus the area occupied Fig.2 The distribution of the areas of heights levels in the northern and southern hemispheres Fig.3 The distributions of the areas heights levels in eastern and western hemispheres of Mars ...
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Ссылки http://selena.sai.msu.ru/Rod/Publications/ms34/MS060.pdf -- 166.4 Кб -- 06.10.2008
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13. SPUTNIK home page
... Average resolution at altitude H=668 km . ... Swath width at H=668 km and inclination of beginning of swath 20.48 degrees . ... Resolution at H=668 км . ... Наименование параметра . ... 1 канале . ... Полоса обзора при H=668 км . ... 1-5 спектральной зоне, не более . ... 1 спектральной зоне . 0,48-0,52 мкм . ... 0,915-0,997 мкм . ... 1-4 канал . ... 1-4 каналов . ... Спектральные характеристики каналов (по уровню 0,5): . ... For more information send a mail to: info@sputnik.infospace.ru . ...
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Ссылки http://sputnik.infospace.ru/ocean_o/engl/ocean_1.htm -- 19.8 Кб -- 21.01.2002
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14. ESO - ESO-MIDAS Releases and Distribution
... Public . Science . ... Science Users Information Science Software ESO-MIDAS jump to navigation jump to content . ... Publications with ESO Data . ... ESO-MIDAS . ... The short statement of the GNU license is included in every MIDAS file; the full text is included as a separate file in the ESO-MIDAS Release. ... Manual pages,installation guides and other documentation are generally released together with the source code and can also be obtained from the ESO-MIDAS ftp account (see below). ...
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Ссылки http://www.eso.org/sci/software/esomidas/midas-distrib.html -- 27.7 Кб -- 10.04.2016
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15. Initial Distributions of Binary Parameters
Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...
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Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node39.html -- 14.1 Кб -- 26.02.1997
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16. Measurement of the dark halo shape in polar ring galaxies
... According to the most popular cosmological paradigm, the greater part of the galaxy mass is accumulated in the dark matter halo. ... The polar ring galaxies (PRGs) reveal external rings or disks of gas, dust and stars rotating in a plane roughly perpendicular to the disk of the central galaxy. ... The shape of the dark halo in the model was chosen so as to achieve the best fit to the observed rotation of both galaxies themselves and their polar rings. ... The SPRC-7 galaxy. ...
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Ссылки http://www.sao.ru/Doc-en/SciNews/2014/DMhalo/ -- 8.9 Кб -- 10.04.2016
[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/2014/DMhalo/ -- 8.9 Кб -- 10.04.2016
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17. The Network Time Protocol (NTP) Distribution
... The Network Time Protocol (NTP) is used to synchronize the time of a computer client or server to another server or reference time source, such as a radio or satellite receiver or modem. ... Information on the NTP architecture, protocol and algorithms can be found in the Further Information and Bibliography page. The Building and Installing the Distribution page presents an overview of the procedures for compiling the distribution and installing it on a typical client or server. ...
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Ссылки http://www.sai.msu.su/~er/xntp/ -- 8.7 Кб -- 21.12.2007
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18. http://www.naic.edu/vscience/schedule/tpfiles/McCandlisstagA2233tp.pdf
... A2233 Date Received: 2006-May-31 23:23:18 Technical Page Proposal Type: General Category : Sub- Category : Observation Category : Total Time Requested: Minimum Useful Time: Prop osal Title: ABSTRACT: Short Astronomy Spectroscopy Galactic 3 Hours 90 minutes Neutral Hydrogen Mapping of the Planetary Nebula M27 We propose to acquire a spatial- velocity data cube of the neutral hydrogen distribution in direction of the the planetary nebula ...
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Ссылки http://www.naic.edu/vscience/schedule/tpfiles/McCandlisstagA2233tp.pdf -- 55.3 Кб -- 15.08.2006
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19. Journal "Peremennye Zvezdy"
2dF Sees Waves of Galaxies . ... The 2dF system measures galaxy redshifts , allowing astronomers to estimate distances to some of the millions of galaxies visible, and hence to make a three-dimensional map of the local universe. ... Detailed analyses of the incoming data indicate that to create such a network of waves, normal baryonic matter must make up only 15 percent of all matter , while all matter must make up only about 30 percent of that needed to make the universe geometrically flat . ...
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Ссылки http://www.astronet.ru/db/varstars/msg/1170644 -- 8.5 Кб -- 02.06.1971
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20. Corrections to the probability distribution
Next: Power of test Up: Basic principles of Previous: Test statistics . In principle, it is possible to compute a value of the statistic for a single frequency and to test its consistency with a random signal ( ). ... The factor N means that there is an increased probability of accepting a given value of the statistic as consistent with a random signal. ... In the command individual descriptions, we often refer to probability distributions of specific statistics. ...
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Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol2/node238.html -- 6.9 Кб -- 23.02.1996
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