Download Calculation of the Brightness of Light: In the Case of by E. M. Feigelson, M. S. Malkevich, S. Ya. Kogan, T. D. PDF

get redirected here By E. M. Feigelson, M. S. Malkevich, S. Ya. Kogan, T. D. Koronatova, K. S. Glazova, M. A. Kuznetsova (auth.)

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Table 8 shows that function III gives a maximum value of ~z) (0 ,9 ,1/J) since to it corresponds maximum y (0). 4), but the values of :r(Z) (0, t ,0) which correspond to them are different. This may be explained by the values ofr 1 /r2 for these functions: the much greater value of r 1 /r2 for function VII leads to the shift of the whole curve of 1(2 )(0, e ,0) toward larger values. <2 )(0,9,0). In a similar way the quantities y(1T) and r 1/ r2 explain the behavior of the curve in Fig. 25 which shows J< 1) ( r• ,e ,1/J) as a function e.

Reflection of Light from the Earth's Surface The effect of reflecting properties of the earth's surface on the magnitudes of intensity can be seen in Tables 9 and 10, in which r(l) (r•,El,l/J) and I~2 >co,e ,l/J) are compared for two different scattering functions and different albedo (relative differences between them are also given). 9 the rate of change of 1(1) and r(2 ) is roughly the same. >co, Reflection from the Earth's Surface Sect. l, 5 =tl" 0, 2 Fli YJIJ. Ylll 0 ,J(J 0 fjtJO 8 Fig. 26 50a Fig.

To a lesser extent, although they decrease somewhat, so that the effect of anisotropy of scattering in the case of downward radiation is not considerably reduced. The above role of the reflecting properties of the underlying surface, which manifests itself in a reduction in the effective anisotropy, is connected with the assumption that Lambert's law holds. The effect of the albedo on the distribution of l(l) ( T , e , 'If;) and 1(2 ) ( T , e, 'If;) with height is shown in Fig. 9. at all heights right up to the upper boundary of the atmosphere.

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