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Íà ýòîé ñòðàíèöå ïðèâåäåíû âñå ñòðàíèöû ñåðâåðà www.tesis.lebedev.ru ,êîòîðûå ìû èíäåêñèðóåì. Ïîêàçàíû äîêóìåíòû 39681 - 39695 èç 39695.

[ Â íà÷àëî ] Ïðåä. | 1976 | 1977 | 1978 | 1979 | 1980 | 1981 | 1982 | 1983 | 1984 | 1985

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39681. SphinX press release
... Polish scientists at the Space Research Centre, Polish Academy of Sciences, in Wroclaw, south-west Poland, have constructed an instrument called SphinX (short for Solar PHotometer In X-rays), which is an X-ray spectrophotometer, that will obtain spectra in the energy range 0.5--15 keV in 256 energy channels with frequency of up to 100 times a second. ... SphinX is part of a package of instruments known as TESIS (PI Prof. Sergei Kuzin, Lebedev Institute, Moscow). ... Space Research Centre, . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.tesis.lebedev.ru/info/SphinX_pr.php -- 7.2 Êá -- 01.10.2012
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.tesis.lebedev.ru/ru/info/SphinX_pr.php -- 7.2 Êá -- 01.10.2012
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39682. ÒÅÑÈÑ - ïëàìÿ íà Ñîëíöå
... ÈÇÎÁÐÀÆÅÍÈÅ ÍÅÄÅËÈ NASA HEASARC . Óäèâèòåëüíî êðàñèâîå è ðåäêîå ÿâëåíèå íà Ñîëíöå, çàðåãèñòðèðîâàííîå òåëåñêîïàìè ÒÅÑÈÑ, îïóáëèêîâàíî íà ñàéòå NASA â ðóáðèêå "Èçîáðàæåíèå íåäåëè" . ... Ñòðóêòóðû íà ðèñóíêå íàïîìèíàþò ÿçûêè ïëàìåíè íàä ïîâåðõíîñòüþ Ñîëíöà. ... Ïðèâåäåííîå âûøå èçîáðàæåíèå áûëî ïîëó÷åíî 8 Ìàðòà 2009 ãîäà Ðîññèéñêîé ñîëíå÷íîé îáñåðâàòîðèåé ÒÅÑÈÑ íà áîðòó ñïóòíèêà ÊÎÐÎÍÀÑ-ÔÎÒÎÍ, êîòîðûé áûë çàïóùåí 30 ÿíâàðÿ 2009 ãîäà ñ êîñìîäðîìà Ïëåñåöê íà ñåâåðå Ðîññèè. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.tesis.lebedev.ru/info/sun_flame.php -- 10.2 Êá -- 01.10.2012
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39683. Íà÷àëîñü ôîðìèðîâàíèå íîâûõ ïîÿñîâ àêòèâíîñòè Ñîëíöà
Íàáëþäåíèÿ ðîññèéñêîé îáñåðâàòîðèè ÒÅÑÈÑ 27 ìàðòà 2009 ãîäà â ëèíèè FeIX 171 A . ... Õîòÿ íà ïîâåðõíîñòè Ñîëíöà ñåé÷àñ íåò íè îäíîãî ïÿòíà, è ñ Çåìëè îíî êàæåòñÿ ñîâåðøåííî ñïîêîéíûì, òåëåñêîïàì ÒÅÑÈÑ, âåäóùèì íàáëþäåíèÿ èç êîñìîñà, óäàëîñü ñäåëàòü ïåðâîå îòêðûòèå : ñïóñòÿ äâà ãîäà çàòÿíóâøåãîñÿ ìèíèìóìà íà Ñîëíöå íà÷àëîñü ôîðìèðîâàíèå íîâûõ ïîÿñîâ àêòèâíîñòè. ...  ýòîì æå öèêëå èç-çà çàòÿíóâøåãîñÿ ïî÷òè íà 2 ãîäà ìèíèìóìà ïîÿñ àêòèâíîñòè ïðåäûäóùåãî öèêëà îêàçàëñÿ óæå ïîëíîñòüþ ðàçðóøåí. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.tesis.lebedev.ru/info/new_cycle.php -- 9.7 Êá -- 01.10.2012
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39684. http://www.tesis.lebedev.ru/en/docs/1532.pdf
... The data from the X-ray spectrometer RESIK, gamma spectrometer HELICON, flare spectrometer IRIS, amplitude­temporal spectrometer AVS-F, and X-ray spectrometer RPS-1 have been used to analyze the X- and gamma-ray emission from solar flares and for diagnostics of the flaring plasma. The absolute and relative content of various elements (such as potassium, argon, and sulfur) of solar plasma in flares has been determined for the first time with the X-ray spectrometer RESIK. ... V.D. Kuznetsov et al. ...
[ Òåêñò ]  Ññûëêè http://www.tesis.lebedev.ru/en/docs/1532.pdf -- 827.0 Êá -- 06.12.2011
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39685. http://www.tesis.lebedev.ru/en/docs/1533.pdf
Sun and Geosphere, 2011; 6(1): - 33-35 ISSN 1819-0839 White light corona at different phases of the solar cycle P. V. Stoeva1, A. D. Stoev1, S. V. Kuzin2 1 Space and Solar-Terrestrial Research Institute, BAS, Stara Zagora Department, Bulgaria 2 Lebedev Physical Institute, RAS, Moskow, Russia E-mail: penm@abv.bg, stoev52@abv.bg, kuzin@sci.lebedev.ru Accepted: 12 October 2011 Abstract. ... 33 V. Stoeva, A. D. Stoev, S. V. Kuzin, White light corona at different phases of the solar cycle Fig.1. ...
[ Òåêñò ]  Ññûëêè http://www.tesis.lebedev.ru/en/docs/1533.pdf -- 905.1 Êá -- 06.12.2011
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39686. http://www.tesis.lebedev.ru/en/docs/1379.pdf
... 53, Moscow, 119991 Russia 2 Moscow Physicotechnical Institute, Dolgoprudnyi, Moscow oblast, 141700 Russia Received May 26, 2008 ° Abstract--The relative intensities of Fe XI­Fe XIII lines in the range 176­207 A have been measured for various plasma structures of the solar corona using data from the XUV spectroheliograph of the SPIRIT instrumentation onboard the CORONAS-F satellite with an improved spectral sensitivity calibration. ... 2005, 2007). ... Density measurement based on Fe XIII lines. ...
[ Òåêñò ]  Ññûëêè http://www.tesis.lebedev.ru/en/docs/1379.pdf -- 730.6 Êá -- 23.12.2008
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39687. http://www.tesis.lebedev.ru/docs/1374.pdf
... × ÜÜãØ ÇãêÒ ãäÛâÜ äã^Òââ ÝÞÛÇã,ãÝ ãäêÛ~ÒâÝÛi ÞÒßÒÜêã, êÒÞÒâÝãä. ðÑßÒÒÜÀ äãäëâÝÜÛÒ ßÜã,,ãâÞãØÜÀi Zr/Si-éÛÞÈêã,, ~ë,âê,ÛêÒÞÈÜãâêÈ Û Û^ÛãÜÜfl âêãØÝãâêÈ ÒêÒÝêã Ü ãâÜã,Ò øñû-ßêÛ^À. øãäëâÝÜÛÒ éÛÞÈêã, , Çã~Òß ÛäÑãÜÒ ÞÛÜ ,ãÞÜ âãâê,ÛÞã ~ 40-50% (Þfl éÛÞÈêã, ÑÜãØ êãÞÛÜÀ), âäÒÝêÞÈÜfl Ñ,ÛâÛßãâêÈ äãäëâÝÜÛfl ÇÞÛÑÝ Ý â~ÒêÜãØ. øãäëâÝÜÛÒ éÛÞÈêã, , ,ÛÛßãØ ãÇÞâêÛ âäÒÝê âãâê,ÛÞã (1-2) ç 10-6. ?ë,âê,ÛêÒÞÈÜãâêÈ ÒêÒÝêã âãâê,ÛÞ 0.01-0.1 Ò. Ôåø/éãêãÜ, Û^ÛãÜÜfl âêãØÝãâêÈ Þë~?Ò, ~Òß 109 . ...
[ Òåêñò ]  Ññûëêè http://www.tesis.lebedev.ru/docs/1374.pdf -- 219.5 Êá -- 25.05.2008
[ Òåêñò ]  Ññûëêè http://www.tesis.lebedev.ru/ru/docs/1374.pdf -- 219.5 Êá -- 25.05.2008
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39688. http://www.tesis.lebedev.ru/en/docs/1373.pdf
... Fe XII Fe XII Fe XIII Fe XII .. ... The Fe XII line ° 201.76 A intensity ratio is I (201.74)/I (201.76) = 1.1-2.5 and ° the contribution from the Ar XIII 201.71 A line does ° The Fe XII 201.76 A lineisblended with theFe XII ° 201.74 A (3s2 3p3 2 P1/2 - 3s2 3p2 (1 D) â 3d 2 P1/2 ) line. ... Fe XIII (log T = 6.2). 3s2 3p2 1 D2 - 3s2 3p3d 1 F3 ° = 196.54 A. ° The 196.54 A line is blended with the Fe XII ° 195.64 A(3s2 3p3 2 D5/2 - 3s2 3p2 (1 D)3d 2 D5/2 ) line. ... Fe XIII 203.16 A line is unblended. ...
[ Òåêñò ]  Ññûëêè http://www.tesis.lebedev.ru/en/docs/1373.pdf -- 872.5 Êá -- 25.05.2008
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39689. http://www.tesis.lebedev.ru/en/docs/1376.pdf
... 53, Moscow, 119991 Russia 2 MoscowPhysicotechnical Institute, Dolgoprudnyi, Moscow oblast, 141700 Russia Received June 15, 2004 ° Abstract--We present a catalog of 100 lines in the wavelength range 280­330 A detected by the RES-C spectroheliograph in solar active regions and flares during the SPIRIT experiment aboard the CORONAS-F orbital station. ... The line intensities recorded during the X3.4 (GOES) solar flare of December 28, 2001, are given. ... The Ca XVIII 302.19 A line is observed. ...
[ Òåêñò ]  Ññûëêè http://www.tesis.lebedev.ru/en/docs/1376.pdf -- 413.8 Êá -- 25.05.2008
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39690. FCKeditor
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[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.tesis.lebedev.ru/FCKeditor/editor/fckeditor.html?InstanceName=ttext&Toolbar=Cms -- 6.7 Êá -- 04.04.2007
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39691. http://www.tesis.lebedev.ru/docs/129.pdf
2005, 31, 8, . ... 11) tg esc = Bm /B - 1 bm /b - 1 (8) (11), , 1 l2 b tg2 0 = bm /b - 1 1 = bm - b. (12) l2 tg2 0 (10) : K = K0 sin2 0 1 +b . ... f0 (K0 ) : dN (K0 ,0 ) = N0 f0 (K0 )dK0 2 sin 0 d0 , 31 8 2005 (12), Kesc = K0 bm sin2 0 . ... 2 8 2005 606 , 2.0 () 1.5 1.0 c 0.5 a 4 y 0 2.0 ð 1.5 b 1.0 a 0.5 (·) b , , .. , : -esc N =N 0 esc /2 f ()2 sin d = (31) = N0 l b esc sin d sin2 + bl2 cos2 3/2 . ... K N0 : -esc c F =N 0 0 esc f (K,)KdK2 sin d; (46) 0.8 0.6 l 0.4 0.2 a 0 100 - esc (. (11)), -, . ...
[ Òåêñò ]  Ññûëêè http://www.tesis.lebedev.ru/docs/129.pdf -- 494.7 Êá -- 03.04.2007
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39692. http://www.tesis.lebedev.ru/docs/139.pdf
... 2003). ... RHESSI, (HXR) , HXR- . ... 15) n = n0 1+(bm - b)l2 (15) (1) (14), bl(bm - b) , ME = ME0 1+(bm - b)l2 33 1 2007 (16) 67 ME0 - , : ME0 = np0 Ne0 . ... ME = ME0 1+(bm - b) (18) (17) ME/ME0 6 5 4 a 3 b 2 c 1 1.0 0.8 0.6 I (Ç) a 60 40 20 0 0.2 b c 0.4 0.6 (b- 1)/(bm - 1) 0.8 1.0 0.4 0.2 0 () 100 80 (17), (18) . ... 33 1 2007 5* 68 , 1.0 () 0.8 øãêãÝ HXR-ÛÑÞë~ÒÜÛfl, ç 10-8 éãêãÜÀ â-1 Ý×-1 0.6 0.4 0.2 0 1.0 8 (Ç) 6 a b c 0.8 0.6 l 0.4 0.2 0 a 4 2 b c 0 0.2 0.4 0.6 (b - 1)/(bm - 1) 0.8 1.0 . ...
[ Òåêñò ]  Ññûëêè http://www.tesis.lebedev.ru/docs/139.pdf -- 723.2 Êá -- 03.04.2007
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39693. http://www.tesis.lebedev.ru/en/docs/124.pdf
... Printed in U.S.A. THE MOTIONS OF THE HARD X-RAY SOURCES IN SOLAR FLARES : IMAGES AND STATISTICS Sergey A. Bogachev and Boris V. Somov Astronomical Institute, Moscow State University, Universitetskij Prospekt ... the basis of the Yohkoh Hard X-Ray Telescope ( HXT ) data, we present a statistical study of different types of the hard X-ray ( HXR ) source motions during solar flares ... Type I motion of HXR sources in flares. them, the HXR sources systematically moved during flare. ...
[ Òåêñò ]  Ññûëêè http://www.tesis.lebedev.ru/en/docs/124.pdf -- 639.2 Êá -- 03.04.2007
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39694. http://www.tesis.lebedev.ru/en/docs/126.pdf
... 33, No. 1, pp. 62­71. i Formation of Power-Law Electron Spectra in Collapsing Magnetic Traps S. A. Bogachev 1 1* and B. V. Somov 2** Lebedev Institute of Physics, Russian Academy of Sciences, Leninski i pr. ... It is shown that if the electrons injected into the trap have a power-law spectrum, then their spectrum remains a power-law one with the same slope throughout the acceleration process for both the Fermi and betatron acceleration mechanisms. ... They do not coincide at energies below 20 keV. ...
[ Òåêñò ]  Ññûëêè http://www.tesis.lebedev.ru/en/docs/126.pdf -- 657.4 Êá -- 03.04.2007
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39695. http://www.tesis.lebedev.ru/en/docs/128.pdf
Solar System Research, Vol. ... The Dynamics of High-Temperature Plasma in the Solar Corona according to SPIRIT Observations in Mg XII 8.42 å Line S. A. Bogachev1, S. V. Kuzin1, I. A. Zhitnik1, A. M. Urnov1, and V. V. Grechnev2 1Lebedev Institute of Physics, Russian Academy of Sciences, Leninskii pr. ... Our analyses of the time variations in emission during a flare suggest that hot plasma is heated by fluxes of accelerated electrons. ... 39 No. 6 2005 the Mg XII SPIRIT images. ...
[ Òåêñò ]  Ññûëêè http://www.tesis.lebedev.ru/en/docs/128.pdf -- 105.9 Êá -- 03.04.2007
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[ Â íà÷àëî ] Ïðåä. | 1976 | 1977 | 1978 | 1979 | 1980 | 1981 | 1982 | 1983 | 1984 | 1985

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