... 50 m, with atmospheric windows at 10 and 20 m, and the FIR extends to a few hundred ... stretching mode of the SiO bond and at 20 m produced by the bending mode of OSiO ...
3. Database of Optical Properties -- Level: subpage
... sphere . 20*x, 10*m . Q ext , Q sca , Q bk , g, ind (TE/TM) . ... inf.cyl. 20*x, 4*alpha, 10*m . Q ext , Q sca , Q bk , g, ind (TE/TM) . ... 20*x = 0.001, 0.01, 0.1, 0.3, 0.5, 1.0, 2.0, 3.0, 5.0, 10.0, ... 10*m = 1.3, 1.7, 1 ...
4. Database of Optical Properties -- Level: subsubpage
... sphere . 20*x, 10*m . Q ext , Q sca , Q bk , g, ind (TE/TM) . ... inf.cyl. 20*x, 4*alpha, 10*m . Q ext , Q sca , Q bk , g, ind (TE/TM) . ... 20*x = 0.001, 0.01, 0.1, 0.3, 0.5, 1.0, 2.0, 3.0, 5.0, 10.0, ... 10*m = 1.3, 1.7, 1 ...
5. http://www.astro.spbu.ru/staff/ilin2/INTAS/P4-MINSK/PUBL/TEXT/avw-ao.ps
... ing time is maximal for R 3 20 m. When the outer carbon volume fraction inside ... carbon-quartz particles if R 3 < 20 m. When increasing the particle radii these di ...
6. http://www.astro.spbu.ru/staff/ilin2/INTAS2/PAP/P2_4.pdf
... In Fig. 12, we show the images of the cavity configuration at wavelengths of = 3 µm, 10 µm, 20 µm, and 250 µm, respectively. ... At wavelength of = 20 µm, the inner part of the core is optically thick. ...
7. http://www.astro.spbu.ru/staff/ilin2/INTAS2/PAP/P5_1.pdf
... Beichman et al. (1979) resolved the 20 µm infrared emission into three individual ... near-infrared emission, were not detected at 20 µm. Therefore, Evans et al. (1989 ...
8. http://www.astro.spbu.ru/DOP/6-SOFT/SPHEROID/1-SPH_old/Q/hom.res
... 20 ... m Cext/(Pi*Rv**2) Csca/(Pi*Rv**2) Cabs/(Pi*Rv**2 ... 20 1.538489E+00 1.538489E+00 -8.242529E-10 TE ...
9. http://www.astro.spbu.ru/staff/ilin2/INTAS2/PAP/P7_3.pdf
... 2 I ~ f 2 3 ~ 3 1 c2, 2 P3Y 0, (20) cos m , cos m , cos m , cos m , (26) (25) 0 m 1l ... 20 M a ml ml a, N a ml 1 k Mmla, The second terms in Eqs. 9 can be represented in ...
10. http://www.astro.spbu.ru/staff/resh/work/df.ps
... Z M 2 M 1 sch (M)dM : Например, параметры функции Шехтера для галактик поля можно взять из [15]: = 4:4 10 3 Мпк 3 , = 1:21, M = 20:60 (H 0 = 65 км/c/Мпк), а для спиральных галактик поля из [16]: = 2:210 3 Мпк 3 , = 1:11, M = 20:37 (H 0 ...