Fig. 3
Effect of the shape model used for the forsterite grains on the peak position and FWHM. Shown as blue crosses is the distribution of hollow spheres (Min et al. 2003) while green asterisks stand for Mie scattering on spherical grains. Both examples are based on the data from Suto et al. (2006) and cover the temperature range from 50 to 295 K. The grain size is 0.1 μm and the black arrow indicates the temperature dependency.
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