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http://hea-www.harvard.edu/ChandraSNR/G000.1-00.1/radio.cgi.
http://hea-www.harvard.edu/ChandraSNR/G000.1-00.1/radio.cgi.
21. References
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Ссылки http://www.astro.spbu.ru/staff/afk/GalChemEvol/Ref_MC.html -- 5.0 Кб -- 19.11.2010
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22. FLR [Oulu]
spaceweb@oulu.fi - last update: 5 January 1999, 1730 UT (RR) . According to ideal MHD wave theory, a plasma can support two basic wave types, i.e., the magnetosonic wave and the AlfvИn wave. In the theory, standing AlfvИn waves can be excited on geomagnetic field lines , forming so called field line resonances (FLR). ... 1996). ... Bellan, P. M., Mode conversion into non-MHD waves at the AlfvИn layer: The case against the field line resonance concept, J. Geophys. Res. ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/SPPHTEXT/flr.html -- 5.0 Кб -- 13.05.2001
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23. Editing a previous command line
. You can edit any previous command from the history list to create a new command. Suppose that command number 23 in the history list is: 23 lpr part[1-4].ps . Do a preview of the command if you are not sure that it is the right one. To change [1-4] to [5-8] use the command: !23:s/[1-4]/[5-8]/ . This will now run the command: lpr part[5-8].ps . Another way to edit commands in the history list is to move up and down the list until you find the command you are looking for and then edit its command line .
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Ссылки http://comet.sai.msu.ru/UNIXhelp/shell/tcsh_hist5.html -- 2.3 Кб -- 17.01.1997
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24. http://hea.iki.rssi.ru/Z-90/style_blue.css~
inputclass { color : black; font-size : 12px; line-height: 11px; font-family :Verdana, Arial , Helvetica ; border-style: solid ; border-width: 1px ; border- color : #a9a9a9;font-variant: small-caps; } .inputclass_required { color : black; font-size : 12px; line-height: 11px; font-family : Verdana, Arial , Helvetica ; border-style: solid ; border-width: 1px ; border- color : #a9a9a9; background- ...
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Ссылки http://hea.iki.rssi.ru/Z-90/style_blue.css~ -- 6.6 Кб -- 27.05.2004
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25. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE6037889-F8A8-40F0-B9DB-354AEDDAD84B%7D
Cosmic ray intensities (left) compared with predictions (right) from IBEX. The similarity between these observations and predictions as evidenced by the similar color regions supports the local galactic magnetic field direction determined from IBEX observations made from particles at vastly lower energies than the cosmic ray observations shown here. The blue area represents regions of lower fluxes of cosmic rays. ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE6037889-F8A8-40F0-B9DB-354AEDDAD84B%7D -- 4.1 Кб -- 10.04.2016
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- http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BACD4B678-F7FD-4CD5-9A0E-28EA3D8EE5D5%7D
- http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBED9CA7E-AB9A-459A-BEA6-20BEF2B7F088%7D
- http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B60D47BC0-5DE0-4383-934B-0796F1DD0805%7D
26. ADASS 2003 Conference Proceedings
... Up: Data Processing Systems . ... At this point it is indispensable to be able to obtain the measurements of reference features in experimental data such as the wavelength calibration lines with a comparable intrinsic accuracy and repeatability. ... An example of such data is shown in Figure 1, a 70 by 50 pixel window around two ``bright'' calibration lines (slit images) with a maximum photon count of 40 in the brightest pixel. ... Figure 1: Typical photon count distribution for two calibration...
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Ссылки http://www.adass.org/adass/proceedings/adass03/P10-10/ -- 14.6 Кб -- 27.08.2004
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27. Population of Galactic globular clusters, figures
... Galactocentric distance dependences of the physical parameters of globular clusters. ... The straight line in (a) is the rms regression. The large circles in (b) show mean masses within narrow R intervals, and the solid lines show the rms regression fits for thick-disk and old-halo (left) and young-halo and corona (right) clusters. The dashed lines in (c) and (d) are upper and lower envelopes drawn by eye. discussion in the text | privious figure | next figure . ...
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Ссылки http://ip.rsu.ru/~marsakov/paper5/p5fg11_1.htm -- 2.2 Кб -- 02.02.2007
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28. Astronomical Catalogues
... 237S (SIMBAD/NED BibCode) ================================================================================ Keywords: Sun: UV radiation - atmospheric effects - Sun: atmosphere - lines: identification Description: An ultraviolet atlas of the solar spectrum with a spectral resolution of 15mA in the region 1948-2000A is presented. ... The wavelength atlas with a list of about 550 lines has been synthesized from data at center of the Sun ({mu}=1) and at {mu}=0.89, smoothed out over an area of 30 arcsec. ...
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Ссылки http://vega.inp.nsk.su/~inest/astrolib/Sun/kursoviki/Model2000/AtmModel/UV/Source.html -- 10.3 Кб -- 26.03.2000
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29. Supernova images - Best of
Supernova Gallery The purpose of the Bright Supernovae web pages is to provide a place where people can find reference images of Supernovae. ... This is an RGB color image of Supernova 2003gs in NGC 936 Credit: Pablo Canadia . Used by permission. (click on image for full resolution) . ... This is an LRGB color image of Supernova 2003cg in NGC 3169 Credit: Pollux observatory . ... Credit: Nick Suntzeff Used by permission. (click on image for full resolution) . ... Credit: AURA/NOAO Image Library . ...
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Ссылки http://www.sai.msu.su/mirrors/isn/snimages/best_img.html -- 18.7 Кб -- 13.02.2011
[ Сохраненная копия ] Ссылки http://www.rochesterastronomy.org/SNIMAGES/best_img.html -- 19.3 Кб -- 10.04.2016
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[ Сохраненная копия ] Ссылки http://www.rochesterastronomy.org/SNIMAGES/best_img.html -- 19.3 Кб -- 10.04.2016
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30. Long description of example illustrating floating with clear
This diagram illustrates the effects of floating a box ("inner") and how its "sibling" is forced below it due to the 'clear' property. A document window is shown, with 8 lines (numbered 1 to 8), each 24px high. Text before the "inner" box flows on lines 1 and halfway on line 2. The "inner" box has been floated to the right and occupies the second half of lines 3 and 4. ... The lines, as they appear in the image, contain: 1 Beginning of body contents. ... Inner contents" is blue. ...
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Ссылки http://crydee.sai.msu.ru/~vab/html.doc/css2/images/longdesc/flow-clear2-desc.html -- 2.5 Кб -- 01.05.1998
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31. JSC Celebrates 40 Years: Gallery
JSC Turns 40 Home | ... Gallery . Johnson Space Center at 40 Years Imagery . ... S65-34635 (3 June 1965) --- Astronaut Edward H. White II, pilot for the Gemini-Titan 4 space flight, floats in zero gravity of space. The extravehicular activity was performed during the third revolution of the Gemini 4 spacecraft. White is attached to the spacecraft by a 25-ft. umbilical line and a 23-ft. tether line, both wrapped in gold tape to form one cord. ... Curator: JSC Web Team | ...
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Ссылки http://www.jsc.nasa.gov/history/jsc40/gallery/S65-34635.htm -- 7.4 Кб -- 08.07.2015
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32. http://xmm.vilspa.esa.es/calibration/find_obs_logz_new.cgi
... rev }; if ( $rev !~ /^\d{4}$/) { &print_obs_log_sum(" Revolution $rev invalid. ... TR /i) { # until end of row push @saved_lines, $lines[$i]; if ($lines[$i] =~ / (\d{2}):(\d{2}):(\d{2})\.\d{2} /) { # RA line my ($cur_ra) = 15 * $1 + $2 / 4.0 + $3 / 240.; if ($cur_ra = $ra1_min $cur_ra = $ra1_max) {$found_ obs = 1;} if ($split) { if ($cur_ra = $ra2_min $cur_ra = $ra2_max) {$found_ obs = 1;} } } $i++; } if ($found_ obs ) { print _found_row($n_hits, @saved_lines); $n_hits++; $found_ ...
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Ссылки http://xmm.vilspa.esa.es/calibration/find_obs_logz_new.cgi -- 11.4 Кб -- 26.01.2011
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33. Texas Survey of radio sources at 365MHz
The Texas survey of radio sources covering -35.5{deg} < {delta} < 71.5{deg} at 365MHz . ... We present the Texas Survey of discrete radio sources between -35.5deg and 71.5deg declination (B1950), which was carried out at 365MHz with the Texas Interferometer during 1974-1983. ... The Texas Survey . ... The sources in the simpler model. ... Right Ascension 1950 . ... field separator . ... Some sources came from Version 6 of the Texas Survey ('TS6' in strp field) or Version 7 ('TS7' in strp field) . ...
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Ссылки http://www.asc.rssi.ru/mdb/stars/8/8042.htm -- 39.0 Кб -- 08.10.1998
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34. Phil Plait's Bad Astronomy: Bad TV
... Bad Astronomy . ... On Sunday, March 23 rd , the television "superstation" TBS aired a show called "Fire From the Sky", yet another in a long line of documentaries about imminent doom from an asteroid collision. ... They aren't kidding when they say it's a matter of global life and death, and it's terrible that there isn't enough money being spent on searching for Earth crossing asteroids. ... Like "Asteroid", one of their animations showed a cloud of asteroids very close to each other. ...
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Ссылки http://www.badastronomy.com/bad/tv/skyfire.html -- 22.1 Кб -- 09.04.2016
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35. The M111 - "On Line"
Previous Editions of the M111: . ... OutReach Training and Program . September Public Night . Welcome all ye weary travelers to a new type of M111 "On Line". ... Back to top.. ... When I logged our last outreach programs I couldn't help but notice that Warren Rupp Observatory is NUMBER FIVE in the worldwide standings in public outreach programs! ... If you'd like to train in astronomy outreach, just contact any of our members and we'll be happy to train you to do public outreach! ...
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Ссылки http://www.wro.org/ras/m111/august2008m111.html -- 16.0 Кб -- 11.09.2008
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36. ASP: Sharing the Universe
... The Sun . Does anyone know how many stars are there in the solar system? Come take a look at the Sun. See that? ... Did you know all the stars you see when you look up are inside our galaxy! ... Did you know that our Sun and solar system were born in a cloud of gas and dust like this. ... We're looking at a place where stars are being born. ... Sharing the Universe is based upon work supported by the Informal Education Division of the National Science Foundation under Grant no DRL-0638873. ...
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Ссылки http://www.astrosociety.org/SharingTheUniverse/wow_tips.html -- 28.5 Кб -- 02.10.2012
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37. Figures and figure captions
Next: About this document Up: Old neutron star distribution Previous: References . Figure: Velocity distribution of young pulsars calculated from statistical modelling of evolution of 50,000 binary systems. ... Figure: Equal density contours for the calculated distribution of old neutron stars (in arbitrary units). Figure: Plot of (solid lines), (long-dashed lines) and (short-dashed lines) for the calculated old neutron star space distribution versus limiting distance of the sample . ...
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Ссылки http://xray.sai.msu.ru/~mystery/articles/old_ns/node14.html -- 4.9 Кб -- 19.08.1996
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38. Figure 1
... The same spectral region is shown in 8 spectra; two bright lines are seen in each: the line of ionized helium on the right, and the line on the left is the Bowen blend, which consists of 6 lines (3 lines of doubly ionized nitrogen and 3 lines of doubly ionized carbon). ... Below the lines, broad contours are shown; these are the discovered super-broad components, one under the helium line, another one under the Bowen blend, and their sum. ... That is why these components are weak. ...
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Ссылки http://www.sao.ru/Doc-en/SciNews/2014/Fabrika/Fig1.html -- 2.5 Кб -- 28.02.2014
[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/2014/Fabrika/Fig1.html -- 2.5 Кб -- 28.02.2014
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[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/2014/Fabrika/Fig1.html -- 2.5 Кб -- 28.02.2014
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39. The Music of the Spheres
... This is combined emission from all the gas clouds circling the black hole, between 0.1 and 10 light years out. ... These are the expanding clouds of gas left behind when a massive star comes to the end of its life and explodes, producing a supernova. ... Also known as the Veil nebula, a vast and beautiful whispy nebula left over from an exploding star. ... The Crab Nebula (120kb). ... Carbon Star (120kb) Red giant stars, surrounded by clouds or carbon dust. ... 3500 K star (64kb) , like Aldebaran. ...
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Ссылки http://www.mso.anu.edu.au/pfrancis/Music/library/index.html -- 7.5 Кб -- 02.10.2012
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