... 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. ...

... gravitational lensing . ... views of mt. maidanak . maidanak lab home page . ... Gravitational Lensing in Astronomy by Joachim Wambsganss . Lectures on Gravitational Lensing by Ramesh Narayan and Matthias Bartelmann . ... ill-posed inverse problems in msu . Inverse Problems (journal) . Journal of Inverse and Ill-Posed Problems . ... Patricia K. Lamm's Home Page . ...

... 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). ...

Upload Information Template for Hobbes.nmsu.edu =============================================== Archive Filename: DeScribe5_ angled _ folder _ icons _1.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 ...

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. ...

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 ? ...

... 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. ...

... 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. ...

... 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? ...

... 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. ...

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 ...

... 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. ...

... 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 rel