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1. Taurid Complex
Orbital intersection . ... Structure of Taurid stream . ... Meteoroid swarm and Taurid fireballs . ... The following four diagrams schematically show four different Taurid orbits and the orbits of Earth and Jupiter. ... The Taurid stream contains particles (small, solid grains) at different stages of their precession cycles. ... The study of when a meteor stream can produce a meteor shower is the study of when precession brings orbits to intersection with Earth, or e.g. with Mars . ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~aac/zetataur.html -- 8.7 Кб -- 19.10.2007
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2. CCF Components
Next: General CCF Components Up: Calibration Access and Data Previous: List of CAL Routines Contents . This section contains descriptions of the structure of CCF constituents. ... The calibration team of the SOC is also providing additional CCF components where required in conjunction with data that were generated with SciSim. ... These CCF components are generated on a need basis and are identical in structure to the real life components. ... Generation from Ground Calibration Data . ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node653.html -- 30.1 Кб -- 20.09.2011
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Еще в разделе: (Показать все результаты (>5442) - xmm.vilspa.esa.es/ )

3. Data Structure
Data in GIPSY is stored in so called sets . A set consists of two components: an image component and a descriptor component. These components are stored in separate files, but in GIPSY they are always used together. The image data is stored in a `crystalline' structure with a virtually unlimited (up to 20) number of dimensions. ... Within a set subsets can be defined. ... The figure below shows the possible subset types in a three-dimensional set, a `` cube '': . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/gipsy/gds/structure.html -- 4.2 Кб -- 16.01.2009
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4. http://mavr.sao.ru/hq/lizm/conferences/pdf/1987/1987_p27-p30.pdf
... For every level we have plotted the dependence between width and Lande factor and obtained the linear regression parameters: the inclination, the zero Lande factor line width and the correlation. ... Fig. 1. presents a model components, the intensity of which decreases (b) line with 10 and increases (c) to the center of spectral line (the field is 12 k6s). ... Our results show strong dependencies of line width on the level of width measurements. ...
[ Текст ]  Ссылки http://mavr.sao.ru/hq/lizm/conferences/pdf/1987/1987_p27-p30.pdf -- 41.5 Кб -- 24.02.2010
[ Текст ]  Ссылки http://www.sao.ru/hq/lizm/conferences/pdf/1987/1987_p27-p30.pdf -- 41.5 Кб -- 24.02.2010
[ Текст ]  Ссылки http://jet.sao.ru/hq/lizm/conferences/pdf/1987/1987_p27-p30.pdf -- 41.5 Кб -- 24.02.2010
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5. Laboratory of Real Structure of Crystals ISSP RAS
... Laboratory of Real Structure of Crystals . ... Microscopic mechanisms of magnetization reversal of nanostructured magnetic materials (multilayers, spin valves, etc.) ... Dynamical properties of domain walls, Bloch lines and points in ferromagnetics. ... Nonlinear excitations of spin systems localized in domain walls as well as of soliton-like spin waves and their evolutions. Dynamical properties of domain walls in ferroelectrics. ... ISSP RAS © 2006 All rights reserved ...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/lrsc/researchen.html -- 7.1 Кб -- 29.03.2010
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6. IAU 317 Symp. Scientific Rationale
Understanding the early phases of assembly and formation of galaxies is a challenge. ... The IAU symposium 317 at the XXIX IAU GA in 2015 will take place at the verge of a revolution that is brought about by the availability of unprecedent new data, provided by the Gaia satellite, space telescopes (HST, Spitzer) and by a number of large ground-based spectroscopic and photometric surveys of the Milky Way, M31 and external galaxies. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~marnabol/IAU317_Sciencera_04012015.html -- 4.1 Кб -- 09.01.2015
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7. Structure of the Galaxy
Next: Transparency of the Stochastic Up: Model of the Galaxy Previous: Frequency distribution of galactic . ... The parameters of the model resulted from a numerical fitting of various data, such as the observed distribution of the young star population and neutral hydrogen, the density of population II stars in the vicinity of the Sun, the galactic rotation curve and the dynamics and distribution of globular clusters   and dwarf irregular satellites of the Galaxy. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node80.html -- 5.0 Кб -- 04.03.1997
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8. Primary mirror support
... The axial support is provided by 78 air pistons. ... The transverse support is provided by 38 air pistons, supported by cantilevers from the mirror cell, that act on the mirror local center of gravity surface. ... The locations where the transverse mirror support forces should be applied to the mirror are listed in Table 1 and illustrated in Figure 1. ... Figure 1: CAD drawing showing the 2.5-m primary mirror and the locations of the transverse support posts (black) and axial pneumatic pistons (blue...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/SDSS/eng.papers/19980713_1rySupportIII/19980713.html -- 9.9 Кб -- 25.08.1998
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9. MAGION-4 Spacecraft (C2-X)
... The spacecraft of Magion type have been selected as the subsatellites of the Interball project: Magion-4 (C2-X) for the Tail Probe and Magion-5 (C2-A) for the Auroral Probe. ... Magion-4 was produced in the Czech Republic in collaboratrion with Russia, Ukraine, Hungary, Austria and has onboard scientific instruments and sensors designed and built in Czech Republic, Russia, Poland, Hungary, Romania, Bulgaria and Slovak Republic. ... Plasma flow detector VDP-S (Czech Republic, Russia) . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/interball/magion.html -- 8.5 Кб -- 30.08.1999
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/interball/magion.html -- 8.5 Кб -- 30.08.1999
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10. StarView II: A Customizable Query Generation Tool
... Previous: ESO/CDS Data-mining Tool Development Project . ... StarView is the user interface to the Hubble Space Telescope (HST) Data Archive. ... We discuss user interaction with the customizable form, describe the use of Java Foundation Classes in implementing the Model View Controller design pattern, and present design features that allow simple, robust communication with third-party components added at run-time. ... MVC interfaces allow a component to register for data model changes. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass98/kennedybk/ -- 13.0 Кб -- 16.07.1999
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11. Solar system sector, archive 1997
... 1997: . As a result of comprehensive RATAN-600 studies of the prominence on the W limb of the Sun, its instant detailed radiation spectrum in the range from 1.7 to 32 cm (at 39 different wavelengths) was obtained for the first time. ... Own radio emission from the lunar crater Copernicus was registered for the first time at 1.38 and 2.7 cm wavelengths in the RATAN-600 observations of the Moon. This indicates a temperature increase in this crater up to 100K at the depth of 5m. Archive . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/Science/results/ar_solar/res1997.html -- 5.1 Кб -- 10.04.2016
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