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Following the scattering process, the magnitudes of the perpendicular and parallel vibrations may be represented by E o ( , ) and Ek o ( , ), where and are the polar angles describing the direction of the emergence of the radiation (see Figure 32) These waves may be simply represented in terms of a linear transformation of the incident wave, and consequently the relationship can be described in terms of an interaction, much in the same way as is done by the Jones calculus Hence the description of scattering may be written as " # 0 E o ( , ) S ( , ) S2k ( , ) E o , (327) D 1 0 Ek o ( , ) S2 ( , ) S1k ( , ) Ek o

The previous chapter discussed theoretical aspects of fuzzy sets The fuzzy set operators allow rudimentary reasoning about facts For example, consider the three fuzzy sets tall, good athlete and good basketball player Now assume tall (P eter) = 09 and good tall (Carl) = 09 and good

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0 0 where E o , Ek o are the resulting vibrations and S1 , S2 , S1k and S2k are the amplitude scattering functions, dependent on and They comprise real and imaginary parts, in turn dependent on the refractive index, m D m 0 im 00 , of the Q scattering particle, and on its size, a, in relation to the wavelength of the radiation being scattered; normally the size/wavelength relationship is expressed as x D 2 a/ D k a, with 2 / k de ning the wavenumber Generally in an astrophysical situation, the scattering is simple, corresponding to the equivalent of linear dichroism and linear birefringence, there being no circular dichroism and no circular birefringence For mathematical simplicity, it is also convenient to assume that the principal axes of the tensor describing the particle anisotropy coincides with the frame de ned by the and k directions With these assumptions S2 and S2k D 0, and the unity subscript may be dropped leading to a description represented by " # 0 E o ( , ) 0 S ( , ) E o (328) D 0 Ek o ( , ) 0 Sk ( , ) Ek o

= 08

= 05

The amplitude scattering functions may comprise real and imaginary parts so that S D a Sk D a k i b i bk , (329) (330)

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If it is known that a good basketball player is tall and is a good athlete, then which one of Peter or Carl will be the better basketball player Through application of the intersection operator, good good

where the terms a and a k dictate the absorptive effects, their combination describing the extinction; the terms b and b k also describe the linear birefringence According to the type of scattering particle, the values of a , a k , b and b k may be assigned

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= min{09, 08} = 08 = min{09, 05} = 05

sions for the resolved intensity and polarized intensity for Thomson, Rayleigh and more general scattering mechanisms were obtained For Thomson and Rayleigh scattering, and when scatterers and stars are distributed with rotational symmetry, the total polarized ux depends on the inclination, i, of the galactic axis to the line of sight according to a simple sin2 i law By using a method based on spherical harmonics for the more general scattering mechanisms, it was found that the sin2 i law still holds, to a good approximation Not all the polarization generated in galaxies results from scattered starlight by dust For example, Knacke & Capps (1974) made observations in the infrared of the Seyfert galaxy, NGC 1068, making comment that its ultraviolet excess was identi ed as synchrotron radiation after the discovery of linear polarization The expectation that p should increase at wavelengths greater than 1 m, as dilution from stellar radiation becomes less, was qualitatively borne out by observations at 35 and 102 m

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