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1. QSO Absorption Lines and Other Cosmological Probes
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[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/1997/ph410/l22.html -- 12.7 Кб -- 10.03.1997
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Еще в разделе: (Показать все результаты (>503) - zebu.uoregon.edu/ )

2. Magnetic Field Lines
... If at any point on such a line we place an ideal compass needle, free to turn in any direction (unlike the usual compass needle, which stays horizontal--such needles exist, see bottom of page) then the needle will always point along the field line (drawing below). ... Because of this attachment, the behavior of electrified gas ("plasma") in space, a gas of free ions and electrons, is dictated by the structure of field lines: Electric currents, for instance, find it easiest to flow along such lines. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/mirrors/stern/Education/wfldline.html -- 8.6 Кб -- 21.12.2007
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3. The Exploration of the Earth's Magnetosphere"
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[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/mirrors/stern/Education/Slides/8-Trapping.htm -- 2.2 Кб -- 21.12.2007
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/mirrors/stern/Education/Slides/8-Trapping.htm -- 2.2 Кб -- 22.12.2007
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4. Spectral Line Processing and RPFITS files
Next: Spectral Line Processing and Up: Spectral Line Data Reduction Previous: ATCA Spectral Line Correlator . ... The ATCA allows you to observe two frequency setups simultaneously ifsel allows you to load just one of them by setting ifsel=1 or ifsel=2 . ... The RPFITS file does not contain the rest frequency of the spectral line observed, so you need to give this at some stage during data reduction - the earlier the better. The rest frequency can be entered (via restfreq , in GHz) in atlod . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/miriad/userguide/node137.html -- 6.6 Кб -- 10.04.2016
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5. signal processing signal optimization line profile analysis Be stars
... temporal activity in stellar atmospheres and signal processing of spectral data. ... 1) 1996: Found X-ray/UV/optical link of initial outburst event in a Be star. 2) 1996: Resolved radiative transfer problem concerning equal emissions of . singlet triplet lines of HeI lines in Be star spectra. ... 4) Late 1970's: Discovery of a new class of variables (nonradial pulsating B stars). 5) Mid 1970's: Application of Fourier techniques for optimized signal recovery . of spectral line profiles. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~msmith/mscv6.html -- 2.3 Кб -- 06.09.2003
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6. Fabry-Perot Interferometer: Gallery Old
... Here some data observed on the 6m telescope with IFP installed in the OLD focal reducer are presented. ... Mkn 3: velocity field . ... NGC 5252: [OIII] image . ... NGC 5252 was observed 23 Feb. 1998 in the [OIII]5007 emission line with CCD TK1024 as detector. ... We observed the ionized gas velocity fields of the spiral galaxies with two purpose. ... Restored velocity field of NGC 157 in the reference frame rotating with the pattern speed overlaid on the Ha image of the galaxy . ... NGC 4100 . ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/lsfvo/devices/scorpio/galleries/gal_ifp.html -- 9.9 Кб -- 28.12.2007
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/lsfvo/devices/scorpio/galleries/gal_ifp.html -- 9.9 Кб -- 11.09.2010
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/lsfvo/devices/scorpio/galleries/gal_ifp.html -- 9.9 Кб -- 02.10.2012
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7. Line Disciplines and Streams Modules
Most radio and modem clocks used for a primary (stratum-1) NTP server utilize serial ports operating at speeds of 9600 baud or greater. ... In order to reduce these errors, a set of special line disciplines and stream modules can be configured in the Unix kernel. ... Note that not all Unix kernels support line disciplines and of those that do, not all support System V streams. ... There are two line disciplines and a special streams module included in the distribution. ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/~er/xntp/ldisc.html -- 8.3 Кб -- 21.12.2007
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8. EMSAO: Radial Velocities from Emission Lines in Spectra
... Many extragalactic objects for which radial velocities are desired display strong emission lines. ... EMSAO, a companion to the cross-correlation task XCSAO (Kurtz et al. 1992), was written to find emission lines automatically, compute redshifts for each identified line, and combine them into a single radial velocity. ... Figure: This EMSAO Summary page shows line centers and fit information for a night sky spectrum. ... To test EMSAO adequately, a lot of emission line spectra were needed. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/minkd.html -- 11.7 Кб -- 03.11.2000
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9. A 215 to 265 GHz spectral line survey of the Sgr B2 molecular cloud
... The spectrum of the Sgr B2 molecular cloud has been surveyed between 215 and 265 GHz towards 3 positions, the dense cores Sgr B2(N)and Sgr B2(M), and the quiescent core Sgr B2(NW). ... The Sgr B2 molecular cloud, located approximately 100 pc from the Galactic Centre and with a mass of , is one of the most extreme cases among star formation sites ( Lis & Goldsmith (1991) ). ... Of the 3 observed positions Sgr B2(N) has the strongest line emission in most molecular species with a few exceptions. ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/yerac/nummelin/nummelin.html -- 7.9 Кб -- 08.12.2003
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10. Line (ImageJ API)
... java.lang.Object ij.gui.Roi ij.gui.Line . ... public class Line . ... int . ... protected double . ... Constructor Detail public Line (int ox1, int oy1, int ox2, int oy2) . Creates a new straight line selection using the specified starting and ending offscreen integer coordinates. public Line (double ox1, double oy1, double ox2, double oy2) . Creates a new straight line selection using the specified starting and ending offscreen double coordinates. public Line (int sx, int sy, ImagePlus imp) . ...
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/gui/Line.html -- 37.4 Кб -- 02.12.2010
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11. Command Line Examples
... omgchain (omgchain-1.8.1) [?? ... Use command `omgchain` to process the ODF data set in the current directory or to where SAS_ODF has been set to, and to place the product files in the current directory. Use command `omgchain outdirectory=output_directory_path` to process the ODF data set in the current directory or to where SAS_ODF has been set to, and to place the output files into the specified directory. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/omgchain/node19.html -- 3.9 Кб -- 22.10.2008
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12. Detecting lines in the comparison (arc) spectrum
Next: Identify the lines Up: Getting Started Previous: Saving and Loading . The Search window is popped up by clicking on the button in the Main window. The different parameters controlling the SEARCH/LONG command can be updated in this dialog window. The file processed is selecting by clicking on in the Search window, which pops up a file selection list. ... The results verification command PLOT/SEARCH is activated by clicking on the button in the Search window. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node532.html -- 3.3 Кб -- 23.02.1996
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13. Power line filters
The alfa motor controller is inside a huffman box. There a few cables that come out to the motor as well as the ac power line. ... The box was using a corcom 6EF2F power line filter. A preliminary sweep of this filter from 0 to 2 ghz using a synthesize and spectrum analyzer showed that the filter worked well up to about 200 MHz. ... We need to figure a way to improve these filters since many of the devices in the huffman boxes have computers that are running at multiple ghz frequencies. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/hardware/Misc/pwrLineFilt/pwrlinefilt.html -- 2.8 Кб -- 20.01.2012
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14. The AstroStat Slog Blog Archive Off the line
... Archives . ... tutorial] multispectral imaging, a case study . ... Off from papers for bridging two, allow me to talk about something relevant to the cultural difference between astronomers and statisticians. I hope this could generate a series of comments. ... Comment ( RSS ) | ... Facebook, LinkedIn, hi5, etcтАж in addition to personal blogs. ... Many of signal processing researchers are like the statisticians you describe. ... Comments RSS . ... Entries (RSS) and Comments (RSS) . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2008/off-the-line/index.html -- 22.6 Кб -- 01.03.2014
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15. Los Cielos de Am , The darkest sky and the two galactic hemispheres
I was wondering what conditions should be met to have the "darkest" sky .. ... Upon the above publication of the Southern Galactic hemisphere, TunГ Tezel started seeking opportunities to create the Northern counterpart image. ... So, the initial quest of having the darkest possible sky have delivered us these two all-sky images of the two galactic hemispheres as seen from Planet Earth. Zoomable and 'full-screenable' fisheye view of the "darkest sky" Southern Galactic Hemisphere image. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~sguisard/Pagim/darkest_sky.html -- 22.9 Кб -- 18.05.2011
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16. S.P.Korolev RSC Energia - A LINE OF PROSTHETIC APPLIANCES
A LINE OF PROSTHETIC APPLIANCES . ... Drawing upon a high scientific and technological potential of prosthetic research institutions of Moscow and St.-Petersburg, using new materials and processes, with support from the Russian Federation Ministries of Economics and Labor, over a 10-year period RSC Energia has managed to set up production of a wide range of advanced modules, assembly units and components for prosthetic appliances. ... NEWS ARCHIVE | ... Official WEB-site of S.P.Korolev RSC Energia . ...
[ Сохраненная копия ]  Ссылки http://www.energia.ru/english/energia/convert/prosthetic/prosthetic.html -- 11.1 Кб -- 25.06.2010
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17. SKY-MAP.ORG
SKY-MAP.ORG
[ Сохраненная копия ]  Ссылки http://www.sky-map.org/ -- 1.8 Кб -- 27.02.2014
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18. IDLINES: identifying spectral lines
... IDL procedure to display ; a) a region of spectrum , together with a fit , if supplied, ; b) positions and relative strengths (gf or W_lambda) of lines in ; common atomic spectra may be marked in the lower panel. ; c) lines of sleceted atoms are identified in the top panel ; ; Command arguments: ; specfile - character string - name of file containing spectrum (and fit ) ; assumed to be x,y file with 3- ... Assesses lines in linelist by the strength values "listfr". ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~csj/idl/IDL_idlines.html -- 4.6 Кб -- 05.05.2009
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19. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B60D47BC0-5DE0-4383-934B-0796F1DD0805%7D
... The upper panel shows a close-up of a region away from the stripes, where the black lines show tangled magnetic field lines and the red line shows an electron spiraling around one of these lines. Electrons with energies of a trillion electron volts (10^12 eV), corresponding to energies about 7 times lower than the maximum energy reached by the Large Hadron Collider (LHC), are responsible for the X-ray emission seen by Chandra. The middle panel shows a close-up of a faint stripe. ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B60D47BC0-5DE0-4383-934B-0796F1DD0805%7D -- 5.9 Кб -- 10.04.2016
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20. Theoretical Astrophysics
Subject, Problems and Objects of Theoretical Astrophysics. ... Stellar Photospheres, Their Features. ... Physics of Continuous Radiation Absorption in Stellar Photospheres. ... Continuous Radiation Absorption in Stellar Photospheres of Various Spectral Classes. Solar Type Photospheres. ... Characterisics of Absorption Lines. ... Interstellar Absorption Lines, Their Features. ... Physical and Dynamic Features of Interstellar Medium, Which Follows from Observations of Interstellar Absorption Lines. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/courses/teor_astroph_e.html -- 8.7 Кб -- 23.02.2005
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