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http://www.atnf.csiro.au/whats_on/workshops/comp2005/talks/sutherland.pdf.

41. Examples of using the lpq command
. To display the print queue for your default printer: lpq Rank Owner Job Files active joe 483 overheads.ps 2nd sarah 484 /tmp/RFC137 3rd tony 485 report . This displays the print queue for your default printer: the one defined by your PRINTER environment variable. Each job in the queue has a job number. Details are also given about the job's position in the queue and the user's name. To display the print queue for a specific printer: lpq -Ppsmath . This displays the print queue for the printer psmath .
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/UNIXhelp/tasks/lpr4.1.html -- 2.3 Кб -- 17.01.1997
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42. http://selena.sai.msu.ru/Symposium/ant.doc
Swirl distribution on the lunar surface: locations antipodal to the young basins? ... THERE ARE TWO MAIN CLASSES OF HYPOTHESISES OF THE SWIRL ORIGIN: FORMATION OF THE SWIRLS IN THE REGIONS ANTIPODAL TO LARGE IMPACT BASINS (1), AND FORMATION OF THE SWIRLS IN RESULT OF COMETARY IMPACTS (2). ... THEY HAVE NEARLY THE SAME AGE. [pic]FIG. ... On the other hand, there are two cases of absence of correlation between swirl areas and regions antipodal to impact basins (for small swirl formations). ...
[ Текст ]  Ссылки http://selena.sai.msu.ru/Symposium/ant.doc -- 169.5 Кб -- 06.10.2008
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43. Description of SED models
... FTP access the basic models is here . ... Below, we put short descriptions of the used SED models for the photometric redshifts providing by the current server . ... The uniqueness of this model consists in expanding to the near IR (NIR) of Rocca-Volmerange and Guiderdoni's (1988) atlas of synthetic spectra with a revised stellar library, which includes parameters of cool stars. ... Homepage of the GISSEL model). ... Another model used earlier is the model of synthetic spectra of Poggianti (1997). ...
[ Сохраненная копия ]  Ссылки http://sed.sao.ru/sed_E_models.html -- 9.2 Кб -- 12.01.2005
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44. Distribution of the analyzed SEPs with different >100 MeV proton fluxes (J100)
Distribution of the analyzed SEPs with different >100 MeV proton fluxes ( J 100 ) at the microwave flux density plane ' S 9 vs. ... 1) General correspondence takes place between intensities of microwave bursts and proton fluxes - J 100 increases when S 9 and S 15 rise. ... 3) Powerful microwave bursts ( S 9 , S 15 >3000-10000 sfu ) with hard radio spectra ( S 9 < S 15 ) correspond to majority of powerful proton fluxes ( J 100 >10 pfu ). ...
[ Сохраненная копия ]  Ссылки http://www.izmiran.rssi.ru/~ichertok/SEPs_radio/fig4s.htm -- 7.5 Кб -- 22.03.2012
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45. 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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46. (Untitled)
As in the last years, the Ephemerides of Minor Planets for 2015 are prepared by the IAA RAS only in the electronic form. ... Orbital elements of all numbered planets have been determined in IAA all over again on the ground of available observations in the catalog of the Minor Planet Center. ... More detailed information on orbital elements used in the present volume of EMP and their accuracy is given in section "Information on new orbital elements". ... a) information on new orbital elements; . ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user0e42.htm -- 6.6 Кб -- 10.04.2016
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47. Irina Glushneva
... The main field of my investigations is stellar spectrophotometry. As a result of scientific activity of our group spectrophotometric catalog was created including energy distribution data on 900 stars in the range 3200-7600AA and 250 stars in the range 6000-10800AA (Voloshina et al., Spectrophotometry of Bright Stars, ed. I.N.Glushneva, 1982, Moscow, Nauka, in Russian). ...
[ Сохраненная копия ]  Ссылки http://uranus.sai.msu.ru/glush.html -- 2.6 Кб -- 20.07.2009
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48. http://solarwind.cosmos.ru/txt/2011/presentations/Magnetosphere/Bespalov.pdf
... 18941904; Bespalov P.A. Effective saturation of absorption in a plasma magnetospheric maser. In book: Nonlinear Space Plasma Physics, R.Z. Sagdeev -Editor-in-Chief, American Institute of Physics, 1993, p.339-346]. Magnetospheric plasma maser [Bespalov P.A, Trakhtengerts V.Yu., ... In a magnetospheric plasma maser (MPM) the relatively dense magnetised plasma and the conjugate ends of a magnetic trap form a quasioptical resonator for electromagnetic waves. ...
[ Текст ]  Ссылки http://solarwind.cosmos.ru/txt/2011/presentations/Magnetosphere/Bespalov.pdf -- 1629.9 Кб -- 15.04.2011
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49. General information
General Information . ... We'd like to announce the forthcoming IAU Conference: . ... A conference organized by Sternberg Astronomical institute (Moscow, Russia) and Working group "Site-testing Instruments" of the International Astronomical Union on various aspects of site-testing techniques, approaches and results. RUSSIA, Kislovodsk (Caucasus Mineral Waters region), 4-9 October 2010. ... Victor Kornilov, Sternberg Astronomical Institute . ... 3-4 October: Registration and accommodation . ...
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