... The OC "Mir" orbit parametres before the final burns . ... Orbit period (in min) . ... Mean orbit altitude (km) . ... solar F 10.7 flux . ... F 10.7 <= 100 - low level; 100 < F 10.7 < 150 - medium level; F 10.7 >= 150 - high level . Orbit 86328(15) - the first burn bulding the descent orbit  D V 1 =9.3 m/s. After burn altitude H min = 188.2 km, H max = 219.2 km. Orbit 86329(16) - the descent orbit second impulse D V 2 =10.4 m/s. After burn altitude H min = 158.9 km, H max = 218.5 km. ...

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... After all we cannot send a probe to the star Altair to confirm that it is 17 light years away. ... The "Bessel determined that the star 61 Cygni was about ten light years away" Earth goes around the Sun in one year, so in six month it is in the opposite position in its orbit. ... In 1838 Bessel determined that the star 61 Cygni had a parallax of 0.314 arcseconds and therefore the star was about ten light years away (today the distance is more precisely measured to be 11.4 light years). ...

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Upload Information Template for Hobbes.nmsu.edu =============================================== Archive Filename: DeScribe5_ angled _ folder _ icons _2.zip Short Description : Angled folder icons for DeScribe 5 Long Description : DeScribe 5 logo over David Graser's excellent new eCS angled folder icons release 5 folder Proposed directory for placement: /pub/multimedia/images/ icons Your ...

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• http://crydee.sai.msu.ru/ftproot/pub/comp/os/os2/hobbes/text-archives/DeScribe5_angled_folder_icons_1.txt
• RELATED WORK
• Index of /ftproot/pub/comp/os/os2/hobbes/text-archives

Multichannel Flare Spectrograph . ... phi - the angle between the green vertical line passing through the solar disk image and the violet radius vector "r" of the object located at the center of the spectrograph slit- red cross. positive - clockwise, negative - counterclockwise . ... mx = x coordinate of the coelostat main mirror . ... x : carthesian solar coordinate alog axis parallel to solar equator (in arcsec) . y : carthesian solar coordinate alog axis parallel to solar axis (in arcsec) ...

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• Maidanak Lab page
• Список публикаций Пасынка С.Л.
• jg0007

Crystals of Siberia Solutions for laser systems CRYSTALS of SIBERIA Ltd. ... LBO crystal, SHG Dimensions: 8 mm(W) x 8 mm(H) x 25 mm(L) Cutting angle: Theta: 90 degrees Phi: 11.6 degrees Anti-reflection Coating: DBAR@1064+532 nm both sides Quantity: 1 element Price: $2070 per element Item 2. ...

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• http://vega.inp.nsk.su/~inest/book/LS/LBO_BBO.pdf
• http://vega.inp.nsk.su/~inest/book/LS/KTP.pdf

profile expand 1.001 echo enter filename [.prof omitted] define file ? data $file.prof echo enter axis [1: major 2: minor] define axis ? ... if($axis==1){ lines 102 202 define colu (9+$angle) }else{ lines 2 202 define colu (1+$angle) } read r 1 read prof $colu if($axis==2){ set r=r*3/0.26 } set prof_aux=prof if(prof>0) set mag=2.5*lg(7888)-2.5*lg(prof_aux) set r=r if(prof>0) echo smooth [0:n 1:y] define ism ? if($ism==1) { echo enter filter size [pixels] define size ? ...

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• Uranus - Voyager 2
• Triton - Voyager 2
• Neptune - Voyager 2

... 2004. ... Carbonneau P., Dikpati M. Stochastic fluctuations in a Babcock-Leighton model of solar cycle // Astrophys. ... Erofeev D.V. An observational evidence for the Babcock-Leighton dynamo scenario. ... Langcope D.W., Fisher G.H. The effect of convection zone turbulence on the tilt angles of magnetic bipoles // Astrophys. ... Dikpati M., Charbonneau P. A Babcock-Leighton flux transport dynamo with solar-like differential rotation. ... Axial tilt angles of sunspot groups // Solar Phys. 1999. ...

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... RC0302+0454 . RC0308+0454 . ... RC0318+0456 . RC0355+0449 . Radio source parameters . ... R.A.(B1950) Dec.( B1950) Freq. ... MHz] size["] flux[mJy] 03:00:18.17 +04:43:31.3 1425.0 2.0x1.9 85 03:00:19.60 +04:43:47.3 2.3x2.0 72 R.A.(J2000) Dec.( J2000) LAS Sp. ["] index 03:02:55.33 +04:55:10.2 27.2 0.9 03:02:56.77 +04:55:26.1 --------------------------------------------- # R.A.(J2000) Dec.( ... R.A.(J2000) Dec.( J2000) R.A.(B1950) Dec.( B1950) Magn. ...

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... part 2 | ... Part 1 . The new concept of formation and development of the Solar system. ... Thus, the initial pulse of the rotation of a protosolar cloud of the solar system was determined as a result of the diversion of a part of the moment of the rotational pulse of the Galaxy. ... Besides this new approach to the pre-solar system as a system of the destroyed vortex structure, we can understand now a number of other peculiarities of the Solar system's structure. ...

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• Arithmetic excercises in the Solar system

... With increasing amount of the melt the GBs with non-zero contact angle become apparently completely wetted. A geometrical model describing the influence of the amount of the liquid phase on the mean contact angle and the portion of completely wetted GBs has been developed. ... For the GBs completely covered by a liquid phase, the h = 0° value was assigned. ... The apparently completely wetted GBs are characterized by a non-zero contact angle but, nevertheless, are filled with the liquid phase. ...

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• http://www.issp.ac.ru/lsc/files/Rossolenko2007.pdf
• http://www.issp.ac.ru/libm/papers/222.pdf
• http://www.issp.ac.ru/libm/papers/2005-15.pdf

... Spectral density of atmospheric pressure term around the FCN frequency Amplitude modulation of signal a(t ) A(t ) cos(0t 0 ) A(t ) A0 A cos(t ) A0 [1 m cos(t )] MA0 a(t ) A0 cos(0t 0 ) cos[(0 )t (0 )] 2 MA0 cos[(0 )t (0 )] 2 Annual variation of amplitude of S1 tide Semiannual variation K1; P1 1; 1 S1 (t ) A cos 2 f S1t B sin 2 f S1t Amplitude modulation of complex signal P 430 (410; 480) f 1.002324 (1.002439; 1.002083) f modulation (0.000115 0.000241) Pmodulation (8700 6100) 18.6 years? ...

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• Model 05_w_001, all curves
• Model 05_h_05, all curves
• Model 05_w_05, all curves

... The first column shows the kinematical diagrams, where is the angle between the line of sight on the object and the vector of rotation about Z -axis, and V S is objects line-of-sight velocity relative to an observer at rest at the position of the Sun. The straight lines are regression fits, whose slopes yield the subsystem’s rotation rate. The second column shows the relations between metallicity and distance from the Galactic plane. ... privious figure | next figure . ...

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• POWER SPECTRUM OF THE IRREGULARITIES AND IT'S FIXING
• Scientific Directions Achievements

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... Flights Chronology . ... Project History . ISS Russian Segment . Steps of ISS Assembly . Spaceflights Chronology . Chronology of Extravehicular Activity . ISS 45/46 . ... Rocket Space Complexes . ... Launches Chronology . ... Automatic Space Systems . ... HISTORY . ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

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• S.P.Korolev RSC Energia - UNIVERSAL SPACE PLATFORM

... Информация Руководство и преподаватели Еремин Роман Александрович . ... Публикации . ... Eremin R.A. , Kholmurodov Kh.T., Petrenko V.I. и др. ... Eremin R.A. , Kholmurodov Kh.T., Petrenko V.I., Avdeev M.V. Chapter 3. ... Eremin R.A. , Kholmurodov Kh.T., Petrenko V.I., Avdeev M.V. Solute-solvent interaction in nonpolar solutions of oleic acid as revealed by molecular dynamics simulation // Journal of Surface Investigation. ... Еремин Р.А. , Холмуродов Х.Т., Петренко В.И. и др. ...

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• Баринова Елена Витальевна. Публикации
• Теряева Ольга Викторовна. Публикации
• Кравченко Сергей Васильевич. Публикации

Atmospheric influence on the different radio-engineering system functioning . ESTIMATION OF ATMOSPHERIC OPTICAL CHARACTERISTICS AND REMOTELY SANSED IMAGE CORRECTION . ... Direct transmittance estimation results for 12 channels of the spectrometer CHRIS. ... We have managed to develop a direct method of estimating the discrete Normalized Atmospheric Point Spread Function (NAPSF) from available images alone, not using any external sources of information about the atmosphere. ... IRE RAS 1996-20 11 ...

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... He was born in Cholmogory - a village where one generation before him saw the first Russian observatory and Lomonosov was able to use the angle gaude. ... But the atmosphere of Venus was so "rich" that no only during four last years of Lomonosov's life, but even two centuries after his death the astronomers didn't go far away from his investigations. 200 years exactly after "the star year" of Lomonosov in 1961 the Soviet spaceship - the first in the world went to Venus. ...

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• starstimee
• jupitere
• datevste

... Using multipledetector coincidence events in the 100-350 keV energy band, our analysis yields a polarization fraction from this GRB of 98 Б 33%. ... For a source count rate of S , and fractional polarization of s , the expected azimuthal scattering angle () distribution is S dS = [1 - Q s cos 2( - )]. d 2 (1) 2.4. ... Simulated azimuthal scattering angle distribution of 100% polarized photons at 200 keV originating at the GRB position. ...

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• http://hea.iki.rssi.ru/integral06/papers/I32_Kalemci01-14Feb07_17:25:59_color.pdf
• http://hea.iki.rssi.ru/Z-90/arc/21/Oh.key/angles_single_bounce.pdf
• http://hea.iki.rssi.ru/Z-90/arc/24/derishev.pdf

. This is a new popup window - close it when you are done . Submitted by Bernie Volz on 10/19/2006 21:54:12 . Al Takada - Totality - Wide Angle shot . Logon to post a follow-up comment or review comments from others . Copyright (c) Amateur Telescope Makers of Boston, Inc. About Us Contact Us

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Back to Products ] . Borescope Teletube Specifications . ... Tube Diameter, . ... 1.7 . 170 . ... 200 . ... 270 . ... 1.8 meter long D=3.5 mm fiber light guide . ... Type transcript - A-3(30 0 AOV)-27(270 mm long)-40(4 mm diameter) = A32740 . The boroscope teletubes are equipped with a fixed -focus eyepiece about 60 mm long. Optional is focusing eyepiece 70 mm long. ...

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. The frequency of the spectral maximum f m of the gyrosynchrotron emission vs. the power-law index of the electron spectrum calculated according to Dulk & Marsh (1982). Curves are shown for various column densities LNe of accelerated electrons and magnetic field strengths B . The angle between the line of sight and the magnetic field is 45 degree.

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