... 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 ...

... L.V.Zotov , C. M. Bizouard Envelope calculation () () () E() L.V.Zotov , C. M. Bizouard Envelope calculation () () () E() L.V.Zotov , C. M. Bizouard Amplitude model and forecast 3-layer Neural Network with (7, 7, 1) neurons L.V.Zotov , C. M. Bizouard Phase model and forecast 3-layer Neural Network with (7, 7, 1) neurons L.V.Zotov , C. M. Bizouard Phase and amplitude models ~ Chandler ...

... 3 , «random lasers» - . ... ZnO. ... SPIE Optics&Photonics , , -, 2005 3. ... Markushev V.M., Ryzhkov M.V., Briskina Ch.M. Characteristic properties of ZnO random lasers pumped by nanosecond pulses // Appl. ... Markushev V.M., Ryzhkov M.V., Briskina Ch.M., Cao H., Zhong H., Wang S.-W., Lu W. Analysis of ZnO Random Laser Spectra under Nanosecond Pumping // Proc. of SPIE. ... Markushev V.M., Ryzhkov M.V., Briskina Ch.M., Cao H. Spectra of ZnO random lasers under nanosecond pumping // Proc. of SPIE. ...

... САТУРН . Видим?сть Сатурна у 2005 роц?: ... У 2005 р. буде два пер?оди видимост? планети. ... Сатурн з'являтиметься на неб? з настанням темряви; тривал?сть видимост? св?тила зменшуватиметься: на початку кв?тня вона досягатиме 8 год, а наприк?нц? м?сяця трохи перевищуватиме 5 год. ... Сатурн сходитиме все ран?ше, а тривал?сть темно? пори доби зб?льшуватиметься, тому планету можна буде спостер?гати все довше й довше: наприк?нц? серпня понад 2 год, а ще через м?сяць - майже 5 год. ...

... 8, ``Celestial Mechanics'', 2002 Estimation of masses of some minor planets from observations of perturbed bodies O. M. Kochetova Institute of Applied Astronomy, St. Petersburg, Russia The most straightforward method of mass determination of minor planets is the dynamical one which uses the gravitational perturbations produced by minor planet in the motion of other bodies. ... The values of the masses of minor planets (15), (29) and (65) appear to be rather close in both papers. ...

... Провод . ... Провод установочный алюминиевый . Провод установочный медный . Провод установочный медный гибкий . Провод осветительный медный . Провод, шнур соединительный гибкий . Провод монтажный . Провод авиационный . Провод термостойкий . Провод связи . Провод эмалированный ПЭТ-155 и ПЭТв-2 . ... Цена (руб./кг) . ... 112 . ... 109 . ... 108 . ... 102 . 111 . ... 101 . ... 100 . ...

... 28 2009 9 0 0 0 0 : International Satellites for Ionospheric Studies, ISIS-1,2 (1969-1980) ie - 1 9 (1 9 7 9 - 1 9 8 2 ) , H _ t o p, , : Ne=NmF2/e Htop Htop 50 50 ( ) . h 0 5 to p = h 0 5 to p ­ h m F 2 h 0 5 t o p N e 0 5 = 0 .5 N m F 2 : H t o p = 1.3 236 h 0 5 t o p (EISCAT), ISIS1,2 K19 . 4 : Rz= 0, 50, 100, 150 |µ |=0, 10,...,90є - 5 (µ ) = jCjpj(u), j=0,1,2,3,4,5 u = (µ -45)/10 t=0, 6, 12, 18 . ... Rz=100 | ... 200-250 , 800 ISIS1,2 K19 , , , , - ftp://ftp.izmiran.ru/pub/izmiran/SPIM/ ...

SAYH AL UHAYMIR 085, CV3 : . ... CK Toshiko K. Mayeda2, and 3 19, , 119991, Planetary Geosciences In- Sayh al Uhaymir 085, CV3 , , CK . Sayh al Uhaymir (SaU) 085 11 2002. ... SaU 085 Allende Mokoia (0.77), CV , . ... 0.2 1.4 , CV . ... Sayh al Uhaymir (SaU ) 085. ... 20-100 , Cr, , SAYH AL UHAYMIR 085: CK : M.A. . SaU 085 (CAIs), 1 x 1 1.8 x 1.9 . ... CAIs , . SaU 085 FeO , , , , , , FeNi . ... SaU 085 CV3 . ... FeO SaU 085 NiO, CK (0.7-3.3 % NiO ) (. ... SAYH AL UHAYMIR 085: CK : M.A. . ...

... ed1 (1) . ... Max Speed: . ... at which time 'mx.sm.bmstu.ru' had been up for 0:54:46 . Daily' Graph (5 Minute Average) . Max In: . 1960.0 B/s (0.2%) . Average In: . 204.0 B/s (0.0%) . Current In: . 419.0 B/s (0.0%) . Max Out: . ... Average Out: . 841.0 B/s (0.1%) . Current Out: . 1823.0 B/s (0.1%) . Weekly' Graph (30 Minute Average) . ... Monthly' Graph (2 Hour Average) . ... Yearly' Graph (1 Day Average) . ... Incoming Traffic in Bytes per Second . ...

) ¶є p(t)ё ґ µ m Hё ґ µ m Hє Ч ё ґµ mє -1 (t) t 0ё ¶є 2 2 2 2 = - + (+ - - ) (t) , є є є є є Ч 1/ 3є = 0 ¶¶ = 0є ё ё № z = 1100 ё Ѕ є ґ ¶є Ѕјє Ч Ч µ ё N (|0 + |1 )є ё ё № |1 є ё Щ ґz = 1100 µє Ч № ё z = 1100 є № ЅЅє 100 є Ч є 10 є № № ё Te Ѕѕє Ѕїє Ч Ѕє ґµ ґµ He Mpl ё Ч H e p = w ё w = срвьє wЧ є w + 1 = p/ + 1 V () = 4 ln(/)є ё № Ne ґ µ ґµ 60 -5 / PR 5 · 10 ё 0.94 В 0.99 Ѕє є r = PT /PR 0.2 ns = V () = 4 ...

... Read MPEC 2008-X14 Read MPEC 2008-X16 M.P.E.C. 2008-X15 Issued 2008 Dec. ... 703 Catalina Sky Survey. ... 8.20932 +0.02379978 +0.46381603 P 2.32 H 22.6 G 0.15 U 7 Residuals in seconds of arc 081130 703 0.0 0.0 081130 703 0.2+ 0.1 + 081201 648 0.3- 0.0 081130 703 0.0 0.0 081130 703 0.2- 0.1081201 648 0.1 + 0.1 - 1 of 2 12/22/ 2008 8:13 PM MPEC 2008 -X15 : 2008 WK96 http://www.cfa.harvard.edu/ mpec /K08/K08X15.html 081130 703 081130 703 ...

... Bad Astronomy . ... Bitesize Astronomy . ... Here's a question for you: if you were to place the Moon randomly anywhere in the sky, on average, how many stars would it cover up? ... We found that the sky is about 40,000 square degrees . ... The area of a circle is pi * radius^2, so the Moon's area is pi * (1/4)^2=0.2 square degrees. So the number of stars in an area the size of the Moon is 0.15 stars/square degree * 0.2 square degrees=0.03 stars per Moon area. ... 2008 Phil Plait. ...

... 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 ...

. Universal (Greenwich) Time . Accuracy = 0.2 mb ; Resolution = 0.1 mb ; Stability = 0.1 mb/year . 1 Mb = 0.75 millimeter mercury (Hg ; 0°C) = 100 pascal = 1 hectopascal .

RXTE: 01.03.02 - , 2006 2 . 28 2006 . ... 2001), " : " (, , 2003), " " (, 2003,2005), " " (, , 2005), " " ( , , 2005), " " (, , 2006), " " (, 2006), " X-2 +/-1" (, , 2005), 36- COSPAR (, 2006), 11 , (), (), (), , (). ... X-1 (.) ... Revnivtsev ., Gilfanov M., Boundary layer emission and Z-track in the color-color diagram of luminous LMXBs, Astron.Astroph., ... Revnivtsev M., Sazonov S., Gilfanov M., Churazov E., Sunyaev R., Origin of the Galactic ridge X-ray emission, Astron.Astroph., ...

php /* * Backup script on server. ... Connects to the mySQL * database and creates a backup file of the whole database. ... Yes/No? ... It will void your warranty :-D! $ date = date ( mdy-hia ); $filename = $savepath/$dbname-$ date .sql ; if($use_gzip== yes ){ $ filename2 = $ file ; } else { $ filename2 = $savepath/$dbname-$ date .sql ; } if($send_email == yes ){ $fileatt_type = filetype($ filename2 ); $ fileatt_name = .$dbname. - .$ ... BR>"; $message .= "--{$mime_boundary}\n" ." ...

... CCD is a NICMOS 3 HgCdTe Focal Plane Array (FPS) 256x256 CCD . CCD pixel size = 40 m . CCD gain = 4.73 e - /ADU 0.2 (K.Gloria measured in 1994: 4.56 e - / ADU ( see plot here ) . CCD read noise = 110 e - / pixel 20 . ... Pixel scale = 0.48"/pixel @ f/5 (120 arcsec FOV), 0.24"/pixel @ f/10 (60 arcsec FOV), 0.11"/pixel @ f/20 (30 arcsec FOV) all binned 1x1 . ...

Target: Jupiter Date: 2012-11-05 Time : 03:38:10 Telescope: CDK20N Camera: Apogee U16M Filters: griz Exposure time : Satellites: z' at 0.2 seconds full frame Disk: g' at 0.008 seconds 256x256 subframe r' at 0.006 seconds i' at 0.006 seconds z' at 0.20 seconds Observer: John Kielkopf Processing: John Kielkopf ...

An eight-billion-year-old cluster of stars 13,000 light-years from Earth, called NGC 6791, can be seen in the image. ... This particular cluster is called an open cluster, because the stars are loosely bound and have started to spread out from each other. The area pictured is 0.2 percent of Kepler's full field of view, and shows hundreds of stars in the constellation Lyra. The image has been color-coded so that brighter stars appear white, and fainter stars, red. ...

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