Íàéäåíî äîêóìåíòîâ: 24135 (97 ñàéòîâ) ---- Âðåìÿ ïîèñêà: 0.08ñåê. |
Ïîêàçàíû äîêóìåíòû, ñîäåðæàùèå ôðàãìåíòû òåêñòà èç äîêóìåíòà
http://www.issp.ac.ru/lek/zverev/art76-R.pdf.
http://www.issp.ac.ru/lek/zverev/art76-R.pdf.
1. Ýôåìåðèäà Ñàòóðíà 2004ã.
Ñàòóðí â 2004ã. Ïðîòèâîñòîÿíèå 1 ÿíâàðÿ 2004ã. Ñîåäèíåíèå ñ ñîëíöåì - 9 èþëÿ 2004ã. Äàòà Ïð.âîñõ. ... 1 ßíâ 06h41m58.46s +22 24' 55.6 9.033 8.050 -0.5 179.3 Gem 11 ßíâ 06h38m26.98s +22 29' 28.3 9.034 8.067 -0.4 168.8 Gem 21 ßíâ 06h35m07.65s +22 33' 41.1 9.034 8.115 - 0.3 157.9 Gem 31 ßíâ 06h32m12.03s +22 37' 27.0 9.034 8.192 - 0.3 147.0 Gem 10 Ôåâ 06h29m49.86s +22 40' 42.0 9.035 8.295 - 0.2 136.3 Gem 20 Ôåâ 06h28m08.22s +22 43' 24.8 9.035 8.421 - 0.2 125.9 Gem 1 ...
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Ñîõðàíåííàÿ êîïèÿ
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Ññûëêè http://edu.zelenogorsk.ru/astron/planets/satu04.htm -- 4.4 Êá -- 01.10.2012
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Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>136) - edu.zelenogorsk.ru/ )
2. http://hea-www.harvard.edu/~fine/POV/src/dual_towel_rod.pov
declare chrome = texture { pigment { color rgbf 0.5 0.5 0.5 0 } finish { diffuse 0.1 specular 0.5 reflection 0.7 roughness 0.005 metallic } } #declare dual_towel_rod = union { cylinder { 0,0,0 0,0,0.2 1.3 } torus { 1.3 0.1 rotate 90*x translate 0.1 *z } cylinder { 0,0,0 0,0, 0.3 1.15 } torus { 1.15 0.1 rotate 90*x translate 0.2*z } cylinder { 0,0,0 0,0, ...
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Ñîõðàíåííàÿ êîïèÿ
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Ññûëêè http://hea-www.harvard.edu/~fine/POV/src/dual_towel_rod.pov -- 2.8 Êá -- 30.11.2004
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>822) - hea-www.harvard.edu/ )
3. http://www.atnf.csiro.au/research/hypercompact/talks/Titmarsh.pdf
... 4 0.08567 3.83484 8447.35 yes - ¢¢¡¡ ¢¢¡¡ ¢ ¢ ¢¡ ¡ ¢¡ ¡ 0.3 G302.486-00.030 c2h 0.3 G302.486-00.030 hcn 0.3 G302.486-00.030 hnc 0.2 0.2 0.2 Average Intensity (Jy/ beam ) Average Intensity (Jy/ beam ) 0.1 0.1 Average Intensity (Jy/ beam ) 0.1 0.0 0.0 0.0 0.1 0.1 0.1 0.2120 100 80 60 Velocity (km/s) 40 20 0 0.2120 100 80 60 ...
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Òåêñò
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Ññûëêè http://www.atnf.csiro.au/research/hypercompact/talks/Titmarsh.pdf -- 909.3 Êá -- 08.09.2010
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>2560) - www.atnf.csiro.au/ )
4. http://star.arm.ac.uk/~csj/movies/povray/stars.inc
... Armagh Observatory 2001 July */ #declare Shining_Dwarf_Core = sphere{ 0,0,0 , 0.99 hollow on interior{ media{ absorption rgb 0.0 , 0.0 , 0.0 scattering { 5 rgb 1.0 , 1.0 , 1.0 eccentricity + 0.1 } density { spherical color_map{ [0.00 rgb 0,0,0 ] [ 0.05 rgb 0.1 , 0.1 , 0.5 ] [ 0.2 rgb 0.2 , 0.2 , 0.6 ] [ 0.5 rgb ...
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Ññûëêè http://star.arm.ac.uk/~csj/movies/povray/stars.inc -- 6.6 Êá -- 29.03.2002
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>511) - star.arm.ac.uk/ )
5. http://lnfm1.sai.msu.ru/grav/russian/life/chteniya/sagit2008/Tatevyan.pdf
... TRF - TRS. ITRS ITRF. ... TRS 1 TRS 2 X ( 2) = T1, 2 + 1, 2 R1, 2 X (1) IERS, ITRF2000 ITRF2005 Transformation parameters at epoch 2000.0 and their rates from ITRF2005 to ITRF2000 (ITRF2000 minus ITRF2005) T T T D 10 -9 1 2 3 R 1 R 2 R 3 mm 0.1 ± Rates ± 0.3 -0.2 0.3 mm - 0.8 0.3 0.1 0.3 mm - 5.8 0.3 -1.8 0.3 mas 0.000 0.012 mas 0.000 0.012 mas 0.000 0.012 0.40 0.05 0.08 0.05 0.000 0.000 0.000 0.012 0.012 0.012 (ITRF ) 20 40 2 10 9 12 ( ) 3-5 4- 20 3-8 25-30 1 / 1-3 / 10 / x, y z : (c...) : (c... ...
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Òåêñò
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Ññûëêè http://lnfm1.sai.msu.ru/grav/russian/life/chteniya/sagit2008/Tatevyan.pdf -- 830.6 Êá -- 07.02.2008
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
6. Optical constant database - Level: data
. Mg x Fe 1-x O from Henning et al. (1995) . Use our codes to transform the standard data file to another form. Back to paper page . Last modified: 25/09/98, V.I.
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Ñîõðàíåííàÿ êîïèÿ
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Ññûëêè http://www.astro.spbu.ru/JPDOC/PAPERS/HENNING.95/mgfeo.html -- 3.0 Êá -- 19.11.2010
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>125) - www.astro.spbu.ru/ )
7. http://www.astrosociety.org/edu/publications/tnl/76/8lightcurves.pdf
Change in Brightness Kepler 4b 0.0 % - 0.1 %0.12 - 0.2 % 0.14 0.16 0.18 0.02 0.04 0.06 0.08 Transit Light Curves Set 1 Transit Tracks p. 3 2 4 6 8 10 12 14 16 Time (in days ) 18 20 22 24 26 Change in Brightness HAT-P-7b 0.0 % -1.0% -2.0% 0.2 0.4 0.6 0.8 1.2 1.4 1.6 1.8 2.2 2.4 2.6 2 4 6 8 10 12 14 16 Time (in days ) 18 20 22 24 26 Change in Brightness HAT-P-11b 0.0 % -0.5% -1.0% ...
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Ññûëêè http://www.astrosociety.org/edu/publications/tnl/76/8lightcurves.pdf -- 703.1 Êá -- 02.10.2012
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>21) - www.astrosociety.org/ )
8. http://www.sao.ru/hq/katya/NDG/DVD/Talks/Kurbatov.pdf
... 6 5.5 5 4.5 5.5 6 6.5 7 7.5 8 8.5 9 -1.33 -1.34 -1.35 -1.36 -1.37 -1.38 4.5 5 5.5 6 6.5 7 7.5 8 L - [Z] 0.4 0.38 0.36 0.34 0.32 0.3 0.28 4.5 5 5.5 6 6.5 7 7.5 8 L - [Fe] 0.85 0.8 5.5 6 6.5 7 7.5 8 8.5 9 0.95 0.9 M-L 1.05 1 M - M/L 13/14 M = 106.5 Msol 0.3 [Fe/H] 0.2 OB = 2 km/s 0.3 M = 106.5 Msol OB = 8 km/s 0.3 M = 107.5 Msol OB = 8 km/s 0.3 M = 108.5 Msol OB = 8 km/s [Fe/H] 0.2 0.2 [Fe/H] 0.2 [Fe/H] 0.1 0.1 0.1 ...
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Òåêñò
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Ññûëêè http://www.sao.ru/hq/katya/NDG/DVD/Talks/Kurbatov.pdf -- 183.8 Êá -- 24.02.2010
[ Òåêñò ] Ññûëêè http://mavr.sao.ru/hq/katya/NDG/DVD/Talks/Kurbatov.pdf -- 183.8 Êá -- 01.10.2009
Ïîõîæèå äîêóìåíòû
[ Òåêñò ] Ññûëêè http://mavr.sao.ru/hq/katya/NDG/DVD/Talks/Kurbatov.pdf -- 183.8 Êá -- 01.10.2009
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>340) - mavr.sao.ru/ )
9. http://vega.inp.nsk.su/~inest/workbbeam/cbb3.pdf
0.3 =0.11 s=0.03 s/y = 0.7 0.25 matrix model tracking 0.2 0.15 +s 0.1 -s 0.05 0 0 Coherent synchro-betatron mode tunes vs. the beam-beam parameter . Comparison of matrix calculation and tracking with Gaussian distribution in the synchrotron phase space. 0.02 0.04 0.06 0.08 0.1 0.12
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Ññûëêè http://vega.inp.nsk.su/~inest/workbbeam/cbb3.pdf -- 68.3 Êá -- 18.06.2001
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>36) - vega.inp.nsk.su/ )
10. Àñòðîíåò > Ïàðàìåòðû äâîéíûõ ñèñòåì ñ ÷åðíûìè äûðàìè
... Àñòðîíåò | ... Ïàðàìåòðû äâîéíûõ ñèñòåì ñ ÷åðíûìè äûðàìè . ... Ïðèìå÷àíèÿ ê òàáëèöå: P - îðáèòàëüíûé ïåðèîä, - ôóíêöèÿ ìàññ îïòè÷åñêîé çâåçäû, M X , M V - ìàññû ÷åðíîé äûðû è îïòè÷åñêîé çâåçäû, ñîîòâåòñòâåííî, V pec ïåêóëÿðàÿ ëó÷åâàÿ ñêîðîñòü öåíòðà ìàññ äâîéíîé ñèñòåìû. ... Ïóáëèêàöèè ñ êëþ÷åâûìè ñëîâàìè: êàíäèäàòû â ÷åðíûå äûðû - äâîéíûå çâåçäû - ðåíòãåíîâñêèå èñòî÷íèêè - ÷åðíûå äûðû . Ïóáëèêàöèè ñî ñëîâàìè: êàíäèäàòû â ÷åðíûå äûðû - äâîéíûå çâåçäû - ðåíòãåíîâñêèå èñòî÷íèêè - ÷åðíûå äûðû . ...
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Ñîõðàíåííàÿ êîïèÿ
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Ññûëêè http://www.astronet.ru/db/msg/1176977 -- 33.4 Êá -- 20.05.2002
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>5365) - www.astronet.ru/ )
11. SAI OCL Catalog SAI 8
. Home . Structure of Data . Description . Catalog . Publications . VO . ÞÁ 2000 . 00:40:08.8 . ÞÄ 2000 . +61:34:03 . l . 121.588 . b . -1.275 . diameter . 3.0' . (m - M) 0 . 14.28 0.2 . distance . 7200 700 pc . E(B - V) . 0.3 0.11 . log(t) . 9.15 0.1 . (J, J-H) isochrone VOTable . 2MASS data VOTable . IPHAS IDR data VOTable . Developed by the Team . Send us your questions or feedback
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Ññûëêè http://ocl.sai.msu.ru/catalog/sai_8/ -- 7.5 Êá -- 09.04.2016
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>63) - ocl.sai.msu.ru/ )
12. Laboratory 235. Homepage
... We are developing arrays of antenna-coupled TES direct detectors of 1.0 – 0.2 mm waveband region with the final purpose to create a prototype of supersensitive arrays which can be used in imaging radiometers for future space missions. It is well known that the use of transition edge sensor (TES) bolometers at very low transition temperatures (~ 0.3 - 0.1 é) is one of the most promising ways to achieve appropriate sensitivity of radiometers for submillimeter astronomy. ...
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Ñîõðàíåííàÿ êîïèÿ
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Ññûëêè http://www.cplire.ru/html/lab235/index.htm -- 3.3 Êá -- 09.09.2008
Ïîõîæèå äîêóìåíòû
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>224) - www.cplire.ru/ )
13. http://www.iki.rssi.ru/conf/2009elw/presentations/presentations_pdf/session3/Berezhnoy_ELW.pdf
Impact Produced Exosphere of Europa A.A. Berezhnoy Sternberg Astronomical Institute, Moscow, Russia Equilibrium chemical composition of the impact-induced cloud 0.5 0.45 0.4 0.35 0.3 0.25 0.2 0.15 0.1 3000 3500 4000 T, K 4500 OH H2 5000 O 5500 H H2O Q 0.0045 0.004 0.0035 0.003 0.0025 0.002 0.0015 0.001 0.0005 0 2000 Na NaO H NaO 3000 T, K 4000 5000 1.E-01 2000 Q 1.E-02 1.E-03 1.E-04 T, K 2500 CO 3000 ... Previous detection of cometary impacts on Europa is very tentative. ...
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Òåêñò
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Ññûëêè http://www.iki.rssi.ru/conf/2009elw/presentations/presentations_pdf/session3/Berezhnoy_ELW.pdf -- 51.1 Êá -- 02.03.2009
[ Òåêñò ] Ññûëêè http://www.cosmos.ru/conf/2009elw/presentations/presentations_pdf/session3/Berezhnoy_ELW.pdf -- 51.1 Êá -- 02.03.2009
Ïîõîæèå äîêóìåíòû
[ Òåêñò ] Ññûëêè http://www.cosmos.ru/conf/2009elw/presentations/presentations_pdf/session3/Berezhnoy_ELW.pdf -- 51.1 Êá -- 02.03.2009
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>200) - www.cosmos.ru/ )
14. Traffic Analysis for ge-0/0/3 -- arcrt1
... arcrt1.arcetri.astro.it in . ... ge-0/0/3 Fibra GARR . ... ge-0/0/3 . Max Speed: . ... at which time 'arcrt1' had been up for 36 days, 1:42:07 . Max . Average . Current . ... 5324.5 kb/s (0.5%) . 4933.4 kb/s (0.5%) . ... 3251.4 kb/s (0.3%) . ... 4396.4 kb/s (0.5%) . ... 1298.7 kb/s (0.1%) . 757.9 kb/s (0.1%) . ... 556.4 kb/s (0.1%) . ... 1292.7 kb/s (0.1%) . ... 4451.3 kb/s (0.5%) . ... 2698.6 kb/s (0.3%) . 1299.4 kb/s (0.1%) . ... Incoming Traffic in Bits per Second . ...
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Ñîõðàíåííàÿ êîïèÿ
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Ññûëêè http://www.arcetri.astro.it/CC/mrtg/arcrt1_ge-0_0_3.html -- 7.8 Êá -- 12.06.2013
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>5272) - www.arcetri.astro.it/ )
15. ÓÒÂÅÐÆÄÀÞ
... DZ *= (+1.2 + 1.7) óãë. ñåê. ...  òå÷åíèå 40 ìèí. òåëåñêîï ñîïðîâîæäàë îáúåêò òîëüêî ïðîãðàììíûì âåäåíèåì (îáëà÷íîñòü) è ïðè ïîÿâëåíèè îáúåêòà íàáëþäàòåëü ââåë ïîïðàâêè êîððåêöèè (+ 0.1 è - 0.3 ) óãë. ñåê., íî äàæå è ýòè ïîïðàâêè áûëè óñòðàíåíû ñëåäóþùåé êîððåêöèåé ( ñì. ðèñ. 3 è òàáë. 2 è 3 ). ... Îòñþäà ìîæíî ñäåëàòü âûâîä, ÷òî ïðè íàáëþäåíèÿõ ñ ÏÇÑ-êàìåðîé ÏÔ ÁÒÀ íàêîïëåííàÿ îøèáêà ïðîãðàììíîãî âåäåíèÿ ÁÒÀ íå ïðåâûøàåò çíà÷åíèé (0.1 - 0.2) óãë. ñåê., òî-åñòü ˜ 0.1 ðàçìåðà èçîáðàæåíèé (âñå îöåíêè...
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Ñîõðàíåííàÿ êîïèÿ
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Ññûëêè http://mavr.sao.ru/hq/sekbta/Navedenie/spravka.htm -- 300.9 Êá -- 20.08.2013
[ Ñîõðàíåííàÿ êîïèÿ ] Ññûëêè http://www.sao.ru/hq/sekbta/Navedenie/spravka.htm -- 300.9 Êá -- 20.08.2013
[ Ñîõðàíåííàÿ êîïèÿ ] Ññûëêè http://jet.sao.ru/hq/sekbta/Navedenie/spravka.htm -- 300.9 Êá -- 20.08.2013
Ïîõîæèå äîêóìåíòû
[ Ñîõðàíåííàÿ êîïèÿ ] Ññûëêè http://www.sao.ru/hq/sekbta/Navedenie/spravka.htm -- 300.9 Êá -- 20.08.2013
[ Ñîõðàíåííàÿ êîïèÿ ] Ññûëêè http://jet.sao.ru/hq/sekbta/Navedenie/spravka.htm -- 300.9 Êá -- 20.08.2013
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>376) - jet.sao.ru/ )
16. http://hea.iki.rssi.ru/Z-90/arc/21/Oh.key/angles_single_bounce.pdf
Surface Scattering Angle Surface Point Source, Isotropic Emitter into Sphere 1 0.9 0.8 0.7 0.6 P["] 0.5 0.4 0.3 0.2 0.1 0 0 !/4 !/2 Scattering " 3!/4 ! MC: local line center resonant MC: local HG scattering, g=0.0 Analytic HG, g=-1/3
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Òåêñò
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Ññûëêè http://hea.iki.rssi.ru/Z-90/arc/21/Oh.key/angles_single_bounce.pdf -- 28.9 Êá -- 27.12.2004
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>366) - hea.iki.rssi.ru/ )
17. HD 142, HIP 522, HR 6
HD 142 . HIP 522 . ... Ìàññà ( ñîëíå÷íûõ ìàññ ) . ... Ðàññòîÿíèå â ïåðèöåíòðå - 5.37 à.å. Ðàññòîÿíèå â àïîöåíòðå - 8.23 à.å. Ðàäèóñ ýôôåêòèâíîé çåìíîé îðáèòû (ïîêàçàíà çåëåíûì öâåòîì) - 1.7 à.å.  áàçå äàííûõ SIMBAD ñïåêòðàëüíûé êëàññ çâåçäû F7 V. Íà ðàññòîÿíèè 105 à.å. (â ïðîåêöèè íà íåáåñíóþ ñôåðó) íàõîäèòñÿ êîìïàíüîí ìàññîé 0.56 ñîëíå÷íûõ ñïåêòðàëüíîãî êëàññà Ì. Ïîäîçðåâàåòñÿ íàëè÷èå åùå îäíîé ïëàíåòû íà âíóòðåííåé îðáèòå (áîëüøàÿ ïîëóîñü îðáèòû ~0.47 à.å., ìàññà ~0.3 ìàññ Þïèòåðà). ...
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Ñîõðàíåííàÿ êîïèÿ
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Ññûëêè http://www.allplanets.ru/star.php?star=HD%20142 -- 20.8 Êá -- 02.02.2013
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Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>693) - www.allplanets.ru/ )
18. http://www.eso.org/~mhilker/thesis.html
... Full version (including all figures and appendices [3.1 MB]) . Reduced version 1 (except german summary and appendices [2.4 MB]) . Reduced version 2 (except german summary, appendices and figures [0.2 MB]) . ... Figures of Chapter 2 (10 figures [1.4 MB]) . ... Chapter 2 ( Photometry of galaxies in selected CCD fields [1.4 MB]) . ... Chapter 6 ( Summary and Future Work [40 kB]) . Chapter 7 ( Zusammenfassung (German summary) [36 kB]) . Appendix A ( The photometric catalog [65 kB]) . ...
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Ñîõðàíåííàÿ êîïèÿ
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Ññûëêè http://www.eso.org/~mhilker/thesis.html -- 3.9 Êá -- 15.11.2006
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>3075) - www.eso.org/ )
19. http://crydee.sai.msu.ru/ftproot/pub/rec/games/idgames/levels/doom2/a-c/cotl10.txt
Title : Courage 1.0!! ... Author Info : Authors of Courage 0.1 and 0.2. Description : Courage 0.1 gave you 8 levels. ... Additional Credits to : id, and all play-testers. Play Information * Episode and Level # : 22 Levels! Single Player : Yes, primarily! Cooperative 2-4 Player : Yes, if you want to, do levels 15+ on skill UV! Deathmatch 2-4 Player : Not really. ... New Sounds : Nah. ... You MAY distribute this WAD, provided you include this file, with no modifications. ...
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Ñîõðàíåííàÿ êîïèÿ
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Ññûëêè http://crydee.sai.msu.ru/ftproot/pub/rec/games/idgames/levels/doom2/a-c/cotl10.txt -- 2.7 Êá -- 04.11.1996
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
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20. http://curl.sai.msu.ru/mass/download/doc/shtrel_control.pdf
DIMM . ... 100 000 , 2007 2009 . ... S 0.2). ... 1 3 ) , D DIMM. s DIMM s= D r0 5/3 = 5 D 2 · l2,t , Kl,t (1 4 ) 1.0 S a 0.9 0.8 0.7 LE MTF SE MTF S a 0.6 0.5 0.4 0.3 0.2 0 1 2 3 4 5 6 5/3 7 8 9 10 s = (D/r0) . ... Smin > 0.45, Smin < 0.45, - DIMM, 7 - 8 . ... Smin > 0.45 ( ) Smin < 0.45 , . ... Smin > 0.3 7 l / 0.8 0.6 S o t 1.0 0.4 0.2 Dec Nov Oct Sep Aug Jul Jun May Apr Mar Feb Jan Dec Nov Oct Sep Aug Jul Jun May Apr Mar Feb Jan Dec Nov Oct Sep 2008 2009 . ... 8 MASS/DIMM 2007 2009 , , , , . ...
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Ññûëêè http://curl.sai.msu.ru/mass/download/doc/shtrel_control.pdf -- 196.0 Êá -- 03.01.2010
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