Lorentz line parameters (and estimates of their standard deviations) have been empirically derived from measured reflectance data for muscovite mica, an anorthosite, a diopsidic pyroxenite, an almandite-pyrope garnet, and a soda lime glass. These parameters provide a useful starting point for computer calculations requiring optical constants as a function of frequency and are therefore given here. A novel method of fitting the reflectance data by least squares is described in detail, as is the statistical procedure for estimating the standard deviations of the parameters found.
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This resonance was used to help fit the high frequency data. We do not suggest that it represents a true resonance, but as Verleur11 has discussed, it provides appropriate optical constants provided the range of validity is not exceeded.
Table V
Lorentz Line Parameters for Diopsidic Pyroxenite; Range of Validity is
This resonance was used to help fit the high frequency data. We do not suggest that it represents a true resonance, but as Verleur11 has discussed, it provides appropriate optical constants provided the range of validity is not exceeded.
Table V
Lorentz Line Parameters for Diopsidic Pyroxenite; Range of Validity is
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