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41. http://lnfm1.sai.msu.ru/grav/english/lecture/filtering/LabN7.pdf
Laboratory work N7 Low-pass filtering. 1) Generate the signal with two periodic components and high-frequency noise. ... 2) Perform it's filtering with Panteleev filter 0 - h(t) = e 22 0 |t| 2 0 t 0 |t| cos + sin 2 2 , where 0 is a parameter. The frequency response of the Panteleev filter is ^ h( ) = 4 0 . 4 0 + 4 Select the cut-off frequency (by varying 0 ) for filtering out high-frequency periodic component and noise. 3) Plot the initial and filtered signal. ...
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Ссылки http://lnfm1.sai.msu.ru/grav/english/lecture/filtering/LabN7.pdf -- 33.1 Кб -- 25.02.2009
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42. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BDE9464D1-325C-49E6-8A3A-2F90299E3BB5%7D
. This illustration shows the discovery that the outer Milky Way is a really a mixture of two distinct components rotating in opposite directions. The inner component of the Galaxy's halo spins clockwise with the galaxy's rotation at about 50,000 miles per hour. The outer component rotates counterclockwise to the galaxy at 100,000 miles per hour. SDSS-II, Masashi Chiba, Tohoku University, Japan
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BDE9464D1-325C-49E6-8A3A-2F90299E3BB5%7D -- 3.6 Кб -- 10.04.2016
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43. source comment
. Comment on J1130-1449 . There are two dominant components in our image. Comparison with the 15 GHz image of Kellermann et al. (1998) reveals that the western component is brighter at the higher frequency, indicating that the brighter (eastern) component in our image may have a steep spectrum. VLBApls home page . Last modified: 16 Oct 2000
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Ссылки http://www.vsop.isas.ac.jp/VLBApls/J1130-1449.comment.htm -- 1.6 Кб -- 16.10.2000
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44. Tesla: Software
... Tesla . ... NVidia drivers (260.19.12) . ... PGI FORTRAN Accelerator Workstation (1 license) . pgf77 64,32 bit (PGI FORTRAN 77) . pgf95 64,32 bit (PGI FORTRAN 95) . pghpf 64,32 bit (PGI High Performance FORTRAN) . pgprof PGI Profiler . pgdbg PGI Debugger . pg-dbg-gui PGI Debugger GUI . ... NVidia CUDA components (2.3, 3.1) . MPICH components (1.2.7) . ... MPICH2 1.3 . ...
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Ссылки http://www.izmiran.rssi.ru/icc/comp/tesla/soft -- 8.4 Кб -- 09.04.2016
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45. http://www.sai.msu.su/gcvs/gcvs/nl74/74nl_rem.txt
... SB, Porb = 55.9212d. V0745 Cas| ... Component B of the double system observed brighter than in the Hipparcos Input Catalogue. ... The variability may be due to the fainter component. ... Type ELL: is also possible. pi Cas| ... Variability type and spectral type (F2/F3Ib/II) do not agree. ... Variability type and spectral type (F3/F5II) do not agree. ... Variability may be due to component B. VZ Pic| ... Variability may be due to component B. V1377 Ori| ... SB, Porb = 9.073d. V0421 Cep|105091| ...
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Ссылки http://www.sai.msu.su/gcvs/gcvs/nl74/74nl_rem.txt -- 8.0 Кб -- 15.03.1999
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46. Energy Storage
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Ссылки http://zebu.uoregon.edu/1998/ph162/l8.html -- 11.2 Кб -- 02.06.1998
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47. SET OF MAGNETIC AND ELECTRIC FIELD DETECTORS EXO-EM
SET OF MAGNETIC AND ELECTRIC FIELD DETECTORS EXO-EM . ... 3 components measurements of both magnetic and electric fields; . ... wide frequency range (0 - 10000) Hz; . ... ECHO-EM is intended for measurement of a complete vector and three components of both electric and magnetic fields, and transfers the received data to the block of the processing of the information and also in telemetry. ... digital 0.1-20 Hz; . ... frequency band (0.01- 10000) Hz; . ... digital (500 - 1000) Hz; . ...
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Ссылки http://space.univ.kiev.ua/projects/warning/exo-em.html -- 5.5 Кб -- 15.02.2000
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48. http://www.apo.nmsu.edu/arc35m/Instruments/ARCTIC/Development/ImagerPDR/Assembly.pdf
The Instrument · · · · · · Baffling Coa3ngs Assembly Moths Lab Tes3ng Commissioning NA2 Baffle · · The NA2 baffle will need to be modified The baffle will need to be opened up to allow the 10.8' diameter field through Instrument Baffles · There are three knife edged surfaces inside the instrument Entrance port Back of shuIer housing Op3cal Tensioner Coa3ngs · Dewar Main components Nickel plated Stainless steel components either ...
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Ссылки http://www.apo.nmsu.edu/arc35m/Instruments/ARCTIC/Development/ImagerPDR/Assembly.pdf -- 2118.2 Кб -- 05.12.2013
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49. The NMW survey homepage
NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...
50. Vertical Structure, figures
... Velocity allipcoid parameters as functions of heigt above the Galactic disk for the complete sample of F -stars (left) and a young ( t 3 Gyr) metal-rich ( [Fe/H] -0.13 ) group (reght). ... next figure | previous figure . ...
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Ссылки http://ip.rsu.ru/~marsakov/paper2/p2fg3_1.htm -- 3.0 Кб -- 02.02.2007
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51. ASP: Making a Rainbow
Classroom Activity: Making a Rainbow . ... When white light from the Sun or a light bulb passes through a prism, the light splits into its component wavelengths. ... Red, blue, green colored filters - if possible, cut 1x4-inch pieces of the filters for each student . ... Many students have the misconception that filters somehow dye the light a certain color. ... Younger students can draw the rainbow and make up a mnemonic for remembering the order of the colors (such as, ROY G. BIV). ...
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Ссылки http://www.astrosociety.org/edu/publications/tnl/35/rainbow.html -- 11.3 Кб -- 02.10.2012
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52. (Untitled)
The data in the Table on p. 5788 – 5789 embrace estimated parameters for 128 binary systems in near Earth, Mars crossing, main belt and Trojan orbits (more than 90% of corresponding objects are marked in the Table "Minor planet lightcurve parameters" as undoubtedly binary and in other cases as suspected binary). ... The data were presented by P. Pravec (Astronomical Institute, Academy of Sciences of Czech Republic) (see Pravec, P., Harris, A. W., 2007. Binary Asteroid Population. ...
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Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user9gs2.htm -- 2.3 Кб -- 10.04.2016
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53. General space training
... Space flight . Crew training . ... Space camp . ... mastering the theoretical principles of astronautics; . studying the main components of a manned space complex - transporting spacecrafts (of the types "Soyuz", "Shuttle", ASS (Aviation Space System), etc.), orbital complexes (of the ISS (International Space Station) type), launching complex, Flight Control Center (FCC), search and rescue complex; . ... acquiring theoretical knowledge and initial practical skills of work in spacesuits; . ...
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Ссылки http://www.atlasaerospace.net/eng/podgotovka-okp.htm -- 32.0 Кб -- 09.04.2016
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54. The Apache TPF Port
Configuration Files | ... Options | ... This version of Apache includes changes allowing it to run on IBM's EBCDIC-based TPF (Transaction Processing Facility) operating system. ... It is passed to Apache through the ZINET XPARM field since ZINET is the only way to start the server on TPF. A third group of options apply to both the informational displays (ZFILE) and running the server (ZINET XPARM): -d, -D and -f. The rest of Apache's options are either not applicable or are not supported on TPF. ...
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Ссылки http://neptun.sai.msu.su/manual/readme-tpf.html -- 22.1 Кб -- 05.11.2004
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55. Products
... IRPS is the small size infrared photometer with detector cooled by liquid nitrogen . IRPS was designed as the instrument for work with optical systems with angular apertures . ... Multichannel preamplifiers (N*8) are designed for use with IR and mm wave detectors arrays. ... Thermoelectric cooling system is designed for use with IR detectors. ... IR photodetector modules with detectors cooled by LN2. ... Gas cooled radiation shield optical cryostat, IR detectors. liquid nitrogen capacity 1.2 ltr. ...
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Ссылки http://www.mao.kiev.ua/staff/kuzkov/products01.html -- 7.1 Кб -- 24.03.2011
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56. Kholtygin et al., AZh (2006)
Kholtygin A.F., Burlakova T.E., Fabrika S.N., Valyavin G.G., Yushkin M.V. Microvariability of Line Profiles in the Spectra of OB Stars: delta Ori A . ... We have studied variability of the spectral lines of the OB star delta Ori A -the brightest component of the delta Ori triple system. ... However, some of the variable features go outside the band, presumably due to either imhomogeneities in the stellar wind from .Ori Aa1 or non-radial pulsations of the weaker components of the system, Aa 2 or Ab. ...
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Ссылки http://www.astro.spbu.ru/staff/afk/Papers/2006/delOriA06abstr.html -- 3.0 Кб -- 19.11.2010
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57. http://hea.iki.rssi.ru/conf/hea2010/Presentations/24/Balega.pdf
... 2009) 0 Fig.1 · Max-Planck-Institute for Radioastronomy, Bonn , VLBI ESO, COMPONENTS PARAMETERS FROM INTERFEROMETRY · Following S.Kraus et al. ... Using i=105o , we obtain v sini = 32 km/s. BEST MODEL FIT 1OriC 1 · Mass, M · Luminosity, log L · Radius, R · Teff, K · log g · Equatorial rotation velocity, km/s · Magnetic field , G · The time of life, yrs 35.8 5.20 10.0 37000 4.01 5.4 500-1500 150 000 1OriC 2 10.0 4.69 8.2 30000 3.60 96.2 moves to MS 1 OriC ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2010/Presentations/24/Balega.pdf -- 453.0 Кб -- 26.01.2011
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58. Product
. home . product . gallery . contact . RITCHEY-CHRETIEN TELESCOPES . RITCHEY-CHRETIEN OPTICS . ACCESSORIES .
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Ссылки http://www.astrosib.ru/prod.html -- 7.9 Кб -- 07.12.2015
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59. Circular Polarization
Abstract -- The strengths of magnetic fields in interstellar gas clouds are obtained through observations of the circular polarization of spectral line radiation. ... To infer information about these irregularities from the observational data, we develop statistical relationships between the rms values of the irregular component of the magnetic field and spatial variations in the circular polarization of the spectral line radiation. ...
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Ссылки http://www.inasan.rssi.ru/~dwiebe/abstracts/circular.html -- 2.8 Кб -- 27.09.2012
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60. astro-ph
... astro-ph . ... Whitespace-separated words are treated as AND ed. Show 10 50 100 articles per page in Full Compact mode . ... Quasar Variability in the Framework of Poissonian Models . ... It is shown that in this very general framework the well established anti-correlation between variability amplitude and wavelength can only be understood as an effect of an underlying spectral component which remains stable on long time-scales, and is redder than the variable component. ...
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Ссылки http://vo.astronet.ru/arxiv/?get_articles=1&author=Jr -- 12.6 Кб -- 06.02.2013
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