| |
| | Astron. Astrophys. 360, 777-788 (2000) |
 | | Furthermore, the measured angular distributions of the degree of linear polarization for unpolarized incident light is compared with observational data of comets and asteroids in Sect. |
 | | 7 (left panel) the maximum polarization of olivine sample S increases with wavelength, because the polarization contributed by the small particles increases due to more Rayleigh-like scattering, while the polarization contributed by the large particles changes little, because the value of k is very small for olivine. |
 | | Thus, for the Allende sample, the increase in polarization for the small particles is, apparently compensated by the decrease in polarization for the larger particles. |
| aa.springer.de /papers/0360002/2300777/sc4.htm (2040 words) |
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