Aronson J R, Emslie A G
Appl Opt. 1973 Nov 1;12(11):2573-84. doi: 10.1364/AO.12.002573.
Experimental data on the spectral emittance of particulate minerals, obtained using a Michelson interferometer operating between 300 cm(-1) and 1400 cm(-1) are compared with the results of a new theory of the spectral reflectance (emittance) of such materials. The comparisons show that the theory predicts the infrared spectra of minerals quite well both for single substances and mixtures, over the wide particle size range between 0.3 micro and 330 micro. The good agreement suggests that the theory can be used in the application of remote infrared spectroscopy to such problems as the compositional analysis of the surface of a planet.
使用在300厘米⁻¹至1400厘米⁻¹之间运行的迈克尔逊干涉仪获得的颗粒状矿物质光谱发射率的实验数据，与此类材料光谱反射率（发射率）新理论的结果进行了比较。比较结果表明，该理论在0.3微米至330微米的宽粒径范围内，对于单一物质和混合物，都能很好地预测矿物质的红外光谱。良好的一致性表明，该理论可用于将远程红外光谱应用于行星表面成分分析等问题。
