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1. Chandra Ground Calibration Raytrace Database and Simulator
... The Chandra Ground Calibration Raytrace Database and Simulator provides simulations of tests performed on the Chandra X-Ray Observatory's High Resolution Mirror Assembly (HRMA). ... Prior to its July 23, 1999 launch, the Chandra X-Ray Observatory's High Resolution Mirror Assembly (HRMA) underwent extensive ground calibration (Weisskopf & O'Dell 1997) at Marshall Space Flight Center's X-Ray Calibration Facility (XRCF). ... When determining subsystem parameters the XRCF raytrace simulator, . ...
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Ссылки http://www.adass.org/adass/proceedings/adass99/P1-19/ -- 11.9 Кб -- 09.10.2000
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2. Introduction
Next: Observational Zoo of Binaries Up: No Title Previous: Contents . In the early 1980s, our understanding of binary star evolution љ based on the pioneer work by Paczynski (1971)[ 150 ], Tutukov and Yungelson (1973)[ 195 ], van den Heuvel and Heise (1972)[ 201 ], allowed us to construct a general evolutionary scenario љ which successfully explained the genesis of well-studied normal stars and offered potential explanation for new X-ray sources discovered in space experiments. ...
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Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node2.html -- 13.0 Кб -- 29.03.1997
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3. Appendix B: Map of the Document
Next: Appendix C: RMOH revision history . ... Appendix B: Map of the Document . ... RSOG Pre-Observation Products . ... Observation Summary File (OSF) . GRT (Ground Radio Telescope) Schedule Files . ... Data Processing Log (DPL) . Partial Correlator Input Log . ... JPL/DOTS Monitor Data File (MDF) . ... Ground Radio Telescope (GRT) Products . ... GRT Log File . ... Mission Element FTP sites . Mission Element FTP Directory Structures . ... Penticton Correlator FTP Directory Structure . ...
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Ссылки http://www.asc.rssi.ru/RadioAstron/documents/rmoh/eng/amapdoc.htm -- 8.5 Кб -- 22.05.2001
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4. DOK-2 Results Page
The study of energetic particles acceleration and transport within the magnetosphere and on its boundaries is the main goal of DOK-2 experiment on Auroral Probe in a frame of INTERBALL project. ... DOK-2 uses two pairs of energetic particle telescopes . ... This information is available only during the most informative Real Time mode of DOK-2. ... Full 56-57 channel spectra accumulated during time intervals from 10 s to 1464 s depending on a particle intensity. ... For this time interval: . ...
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Ссылки http://www.iki.rssi.ru/auroral/dok2.htm -- 9.9 Кб -- 28.11.1996
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/auroral/dok2.htm -- 9.9 Кб -- 28.11.1996
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[ Сохраненная копия ] Ссылки http://www.cosmos.ru/auroral/dok2.htm -- 9.9 Кб -- 28.11.1996
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5. ENERGETIC PARTICLE EXPERIMENT DOK-2
ENERGETIC PARTICLE EXPERIMENT DOK-2 . ... Due to much higher energy, angular and time resolution, better separation of electrons and ions it is expected that DOK-2 experiment will allow to re-examine in more details energetic particle population and related processes in magnetosphere regions covered by the spacecraft orbit. ... Thin foil in front of detector absorbes protons with energies E<400 keV so this detector measures electron spectrum in 20 - 420 keV range. ... Energy values, keV . ...
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Ссылки http://www.iki.rssi.ru/interball/dok.html -- 12.3 Кб -- 30.10.1996
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6. Abstract
Proceedings of the Particle Physics and Early Universe Conference (PPEUC). ... TESRE, Consiglio Nazionale delle Ricerche, Via Gobetti 101, 40129 Bologna, Italy . Dip. Fisica, Universit? di Roma TRE, Roma, Italy . ... Observations will take advantage of the exceptional dryness and stability of the atmosphere on the high Antarctic Plateau, at Dome C. The first run of observations was performed in December 96 -- January 97 at the Italian-French site, Concordia, at Dome C (Antarctica). ...
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Ссылки http://www.mrao.cam.ac.uk/ppeuc/astronomy/papers/valenziano/valenziano.html -- 5.1 Кб -- 22.12.2007
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7. Experimetn COLD: Introduction
Experiment COLD . ... JSEC Astronomy . ... The entire project was called "Experiment Cold". ... The best radiometer (in terms of fluctuation sensitivity) known to us, based on a parametric amplifier with a closed-cycle helium cooling system, was used in the experiment; measures were taken to "cool" the radio telescope itself; and a method of controlling the numerous sources of interference was carefully thought out. ...
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Ссылки http://mavr.sao.ru/hq/CG/cold/introduc.htm -- 5.0 Кб -- 24.02.2010
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/CG/cold/introduc.htm -- 5.0 Кб -- 24.02.2010
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/CG/cold/introduc.htm -- 5.0 Кб -- 24.02.2010
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[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/CG/cold/introduc.htm -- 5.0 Кб -- 24.02.2010
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/CG/cold/introduc.htm -- 5.0 Кб -- 24.02.2010
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8. Introduction
Next: Method Up: Image Restorations of High Previous: Image Restorations of High . Astronomical images are commonly taken with the intent of making photometric measurements of objects in the field. For pre-COSTAR HST images, the question then arises: should these measurements be made on the original or on the restored image? When the objects of interest are stellar, we might intuitively expect that higher accuracy will be achieved using the restored image. ...
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Ссылки http://www.stsci.edu/stsci/meetings/irw/proceedings/lucyl.dir/section3_1.html -- 5.0 Кб -- 18.04.1994
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9. LHPP ISSP RAS
... High-pressures experiments are mostly aimed at studying phase transformations in solids, synthesising new phases and studying their composition, crystal and magnetic structure, physical and thermodynamical properties. ... The specific feature of investigations at LHPP that distinguishes it from most other high-pressure laboratories is combining in situ measurements with studies at ambient pressure of new high-pressure phases fixed by quenching to liquid nitrogen temperature. ...
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Ссылки http://www.issp.ac.ru/lhpp/indexen.html -- 9.7 Кб -- 03.04.2014
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10. Mirror baffle measurements
... Secondary Baffle . ... The outside diameter of the tip of ring 5 (the secondary baffle tip) was 1285.7 mm with a range of 0.8 mm p-v. The specifications were 1284.6 and 7.6 mm respectively. ... The outside diameter of the base of ring 5 was 1273.4 mm with a range of 2.0 mm p-v. The specifications were 1272.1 and 8.1 mm respectively. ... The inside diameter of the tip of ring 19 (the primary baffle tip) was 857.7 mm with a range of 0.8 mm p-v. The specifications were 858.0 and 8.6 mm respectively. ...
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Ссылки http://www.apo.nmsu.edu/Telescopes/SDSS/eng.papers/19970703_MirrorBaffles/19970703.html -- 10.2 Кб -- 19.05.1998
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11. Package: construct
These routines are meant to provide a high level mechanism to manage the construction of data. ... Create a management object for creating array data. construct_array_destroy_manager . Destroy a management object for creating array data. construct_array_select_algorithm . ... Construct an array. ... KConstructArrayManager construct_array_create_manager (KListWidget listw, void (*change_name) (), void *info) . ... void construct_array_create_data (KConstructArrayManager manager, CONST char *name) . ...
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Ссылки http://www.atnf.csiro.au/computing/software/karma/lib/construct.html -- 5.9 Кб -- 25.12.2007