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http://edu.zelenogorsk.ru/astron/planets/merc11.htm.
http://edu.zelenogorsk.ru/astron/planets/merc11.htm.
1. Galactic SNRs: FRAMESET list
... The current SNR catalogue is at http://www.mrao.cam.ac.uk/surveys/snrs/ Jump to l =360œ . 1st quadrant: G0.0 + 0.0 G0.3 + 0.0 G0.9 + 0.1 G1.0 - 0.1 G1.4 - 0.1 G1.9 + 0.3 G3.7 - 0.2 G3.8 + 0.3 G4.2 -3.5 G4.5 +6.8 G4.8 +6.2 G5.2 -2.6 G5.4 -1.2 G5.5 + 0.3 G5.9 +3.1 G6.1 + 0.5 G6.1 +1.2 G6.4 - 0.1 G6.4 +4.0 G6.5 - 0.4 G7.0 - 0.1 G7.2 + 0.2 G7.7 -3.7 G8.3 - 0.0 G8.7 -5.0 G8.7 - 0.1 G8.9 + 0.4 G9.7 - 0.0 G9.8 +0.6 G9.9 -0.8 G10.5 - 0.0 G11.0 - 0.0 G11.1 -1.0 G11.1 -0.7 G11.1 + ...
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Ññûëêè http://www.mrao.cam.ac.uk/projects/surveys/snrs-2006/snrs.f_list.html -- 18.0 Êá -- 10.04.2016
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>2020) - www.mrao.cam.ac.uk/ )
2. Îáùàÿ Àñòðîíîìè÷åñêàÿ Êîíôåðåíöèÿ - Ïîêàçàòü ñîîáùåíèå îòäåëüíî - Õâîñòàòûå
Òåìà : Õâîñòàòûå ãîñòüè 16 (êîððåêöèè îðáèòû) .. Ïîêàçàòü ñîîáùåíèå îòäåëüíî . ... Ñîîáùåíèé: 19,465 . Re: Õâîñòàòûå ãîñòüè (êîððåêöèè îðáèòû) .. ... Ýëåìåíòû îðáèòû êîìåòû C/2011 W3 (Lovejoy): . ... Îòïðàâèòü ëè÷íîå ñîîáùåíèå äëÿ Silvester . Íàéòè åùå ñîîáùåíèÿ îò Silvester . ...
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Ññûëêè http://www.starlab.ru/showpost.php?p=436760&postcount=805 -- 24.3 Êá -- 12.04.2016
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3. 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
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>788) - star.arm.ac.uk/ )
4. http://hea-www.harvard.edu/~pgreen/AGASCupdate/numspoilers2.sort
... MAGin-MAGspoiler #Spoiled Input Stars -5.7 1 -5.2 1 -5.0 1 -4.6 1 -4.4 1 -4.2 2 -4.1 1 -4.0 2 -3.9 2 -3.8 1 -3.7 2 -3.6 3 -3.4 1 -3.3 1 -3.2 2 -3.1 2 -3.0 2 -2.9 1 -2 ... .7 2 -2.6 3 -2.5 1 -2.4 5 -2.3 5 -2.2 5 -2.1 3 -2.0 4 -1.9 2 -1.8 4 -1.7 11 -1.6 4 -1.5 7 -1.4 11 -1.3 8 -1.2 15 -1.1 8 -1.0 8 - 0.9 18 - 0.8 12 - 0.7 19 - 0.6 15 - 0.5 14 - 0.4 17 - 0.3 22 - 0.2 12 - 0.1 18 0.0 13 0.1 19 0.2 23 0.3 11 0.4 15 ...
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Ññûëêè http://hea-www.harvard.edu/~pgreen/AGASCupdate/numspoilers2.sort -- 3.0 Êá -- 27.06.2000
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>1038) - hea-www.harvard.edu/ )
5. http://www.mso.anu.edu.au/pfrancis/simulations/barges_light.py
from __future__ import division from visual import * scene = display(range=(3.0,3.0,3.0),width=1300,height=800,forward=( 0.2 ,-0.3,-1.0)) water = box( pos =(0,- 0.1 , 0.0 ), length=10, width=3, height= 0.1 , color =( 0.1 , 0.2 ,1.0)) alength = 2.0 theta = 0.1 pos1 = vector (0,0,0.6) barge1 = box( pos = pos1, length = 2, width = 0.5, height = 0.1 , color =(0.6,0.4, 0.2 )) x1 = arrow( pos = pos1+ vector (0, 0.1 ,0), ...
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Ññûëêè http://www.mso.anu.edu.au/pfrancis/simulations/barges_light.py -- 5.7 Êá -- 15.04.2014
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>279) - www.mso.anu.edu.au/ )
6. http://lnfm1.sai.msu.ru/~anna/kinem-OB-ass.txt
... with known photometry from the catalog by Blaha and Humphreys (1989) OB-ass. l b r Vr dvr nr mul dml mub dmb nm Nt SGR OB5 0.0 - 1.2 2.4 -15.0 19.0 2 0.1 1.7 0.1 2.2 3 31 SGR OB1 7.6 - 0.8 1.3 -10.0 12.1 37 -1.6 1.2 -1.3 1.0 29 66 SGR OB7 10.7 -1.6 1.4 -6.1 17.1 3 -0.0 0.3 -3.3 0.1 2 4 SGR OB4 12.1 - 1.0 1.9 3.5 10.8 9 - 0.7 1.4 - 0.8 2.5 3 15 SER OB1 16.7 0.1 1.5 -5.0 20.0 17 - 0.7 ...
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Ññûëêè http://lnfm1.sai.msu.ru/~anna/kinem-OB-ass.txt -- 9.2 Êá -- 07.03.2003
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Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>299) - lnfm1.sai.msu.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
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>48) - www.astrosociety.org/ )
8. The supernova remnants (SNRs) radio maps, optical and X-ray images (l=0-360deg)
New SNRs (280-360deg) (Duncan+ 1997) . SNR mag. fields maps (Milne 1987) . ... G000.9+0.1 . ... G016.7+0.1 . ... G033.6+0.1 . ... G059.5+0.1 . ... G304.6+0.1 . ... G318.2+0.1 . ... G323.5+0.1 . ... G332.4+0.1 . ... G335.2+0.1 . ... G338.5+0.1 . ... G348.5+0.1 . ... G351.2+0.1 . ... G354.1+0.1 . ...
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Ññûëêè http://www.sao.ru/cats/~satr/SNR/snr_dir.html -- 29.8 Êá -- 17.01.2002
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Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>692) - www.sao.ru/ )
9. 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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Ññûëêè http://www.atnf.csiro.au/research/hypercompact/talks/Titmarsh.pdf -- 909.3 Êá -- 08.09.2010
Ïîõîæèå äîêóìåíòû
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>9564) - www.atnf.csiro.au/ )
10. Ìåðêóðèé 2009
Ìåðêóðèé â 2009 ãîäó: . ... Íàèáîëüøåå ñêëîíåíèå: 23œ53' - 8 èþëÿ 2009. ... Ô(%) Ñîçâ. 1 ÿíâ 20h07m26.13s -21 49' 38.9 0.3498 1.0775 -0.7 18.8 71.0 Cap 6 ÿíâ 20h29m44.67s -19 44' 09.4 0.3249 0.9508 -0.4 19.2 53.5 Cap 11 ÿíâ 20h39m22.09s -17 49' 10.0 0.3097 0.8194 0.3 16.8 30.3 Cap 16 ÿíâ 20h30m39.65s -16 45' 54.9 0.3093 0.7125 2.2 10.2 8.7 Cap 21 ÿíâ 20h06m33.11s -16 54' 18.2 0.3238 0.6638 4.6 3.4 0.8 Sgr 26 ÿíâ 19h42m40.61s -17 47' 18.9 0.3484 0.6824 2.2 12.1 9.8 ...
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Ññûëêè http://edu.zelenogorsk.ru/astron/planets/merc09.htm -- 7.7 Êá -- 01.10.2012
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>1260) - edu.zelenogorsk.ru/ )
11. Model PSFs
Considerable effort has gone into the modeling of the HST point spread function (PSF), both in order to measure the optical aberrations in support of the WFPC2, COSTAR, and advanced scientific instruments, and to provide PSFs for image deconvolution in the aberrated telescope. ... As a consequence of the under-sampling in the WFPC2, the limiting magnitude attainable in the background limit varies by about 0.5 magnitude, depending on the position of the source within the CCD pixel. ... 0.9 . ...
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Ññûëêè http://www.stsci.edu/instruments/wfpc2/Wfpc2_hand2/ch5_psf6.html -- 117.4 Êá -- 29.08.2000
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>6384) - www.stsci.edu/ )
12. 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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Ññûëêè http://hea.iki.rssi.ru/Z-90/arc/21/Oh.key/angles_single_bounce.pdf -- 28.9 Êá -- 27.12.2004
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>422) - hea.iki.rssi.ru/ )
13. 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
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>33) - curl.sai.msu.ru/ )
14. http://www.wdcb.ru/stp/data/cosmic.ray/G%20L%20E/C044/O/SH221089.AAB
... INTERVAL TD C/S (mb) C/S ALMA-ATA 891022 3600 070000-080000 00 1101.80 681.0 1101.80 0.6 ALMA-ATA 891022 3600 080000-090000 00 1107.48 680.8 1105.89 1.0 ALMA-ATA 891022 3600 090000-100000 00 1112.46 680.6 1109.26 1.3 ALMA-ATA 891022 3600 100000-110000 00 1109.05 680.7 1106.66 1.0 ALMA-ATA 891022 3600 110000-120000 00 1110.33 680.5 1106.34 1.0 ALMA-ATA 891022 ...
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Ññûëêè http://www.wdcb.ru/stp/data/cosmic.ray/G%20L%20E/C044/O/SH221089.AAB -- 14.0 Êá -- 20.06.2005
Ïîõîæèå äîêóìåíòû
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Åùå â ðàçäåëå:
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15. Change history
... offset correction values now read from file . ... offset columns, selected bad pixels & columns, . ... offset correction thresholds now per pixel . ... sigma threshold for offset correction added; . mask rows 1-15 set to bad . ... detailed task description added . ... task description updated . ... description of soft flare screening added . ... new parameters: -set, -withoffsetmap . new algorithm: energy correction calculated . directly from offset maps . ...
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Ññûëêè http://xmm.vilspa.esa.es/sas/7.1.0/doc/epreject/node2.html -- 5.5 Êá -- 15.11.2007
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>2407) - xmm.vilspa.esa.es/ )
16. Ternary metal chalcogenide crystals
. TERNARY METAL CHALCOGENIDE CRYSTALS . By special order we carry out growth of ternary metal chalcogenide crystals: . CdZnS, CdZnSe, CdZnTe , CdSSe, CdSTe, CdSeTe, ZnSSe, ZnSTe, ZnSeTe, CdMnS, ZnMnS and some other . Cd 0.8 Mn 0.2 S single crystal . Cd 0.9 Zn 0.1 Te single crystal . Cd 0.3 Zn 0.7 Se crystal . Cd 0.6 Zn 0.4 Se samples . Zn 0.9 Mn 0.1 S crystal . ZnSe 0.9 S 0.1 :Ni crystal .
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Ñîõðàíåííàÿ êîïèÿ
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Ññûëêè http://www.issp.ac.ru/lpcbc/DANDP/Ternary.html -- 3.8 Êá -- 08.01.2004
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Åùå â ðàçäåëå:
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17. 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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Ññûëêè http://www.astro.spbu.ru/JPDOC/PAPERS/HENNING.95/mgfeo.html -- 3.0 Êá -- 19.11.2010
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Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>166) - www.astro.spbu.ru/ )
18. 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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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
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[ 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
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>615) - jet.sao.ru/ )
19. 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:
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20. http://www.mccme.ru/albio/slides/panteleev.pdf
... The problems of complexity in coagulation: specification 1. ... Numerical experiments Task 1: Activation threshold Final clot density VS activation : model reduction Factor V is activated 7 6 7 6 No factor V activation Fibrin 4 3 2 1 0 0.00 0.02 0.04 0.06 0.08 0.10 0.12 Fibrin 5 5 4 3 2 1 0 0.00 0.02 0.04 0.06 0.08 0.10 0.12 Activation Activation y= Ae ( Bx 1 ) y = Ax Final clot density VS activation : the experiment Fibrin clot density (a.u.) 1.0 0.8 0.6 0.4 0.2 ...
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Ññûëêè http://www.mccme.ru/albio/slides/panteleev.pdf -- 2897.4 Êá -- 09.10.2008
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
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