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Optical mineralogy : ウィキペディア英語版
Optical mineralogy

Optical mineralogy is the study of minerals and rocks by measuring their optical properties. Most commonly, rock and mineral samples are prepared as thin sections or grain mounts for study in the laboratory with a petrographic microscope. Optical mineralogy is used to identify the mineralogical composition of geological materials in order to help reveal their origin and evolution.
Some of the properties and techniques used include:
* Refractive index
* Birefringence
* Michel-Lévy Interference colour chart
* Pleochroism
* Extinction angle
* Conoscopic interference pattern (Interference figure)
* Becke line test
* Optical relief
* Sign of elongation (Length fast vs. length slow)
* Wave plate
==History==
William Nicol, whose name is associated with the creation of the Nicol prism, seems to have been the first to prepare thin slices of mineral substances, and his methods were applied by Henry Thronton Maire Witham (1831) to the study of plant petrifactions. This method, of such far-reaching importance in petrology, was not at once made use of for the systematic investigation of rocks, and it was not until 1858 that Henry Clifton Sorby pointed out its value. Meanwhile, the optical study of sections of crystals had been advanced by Sir David Brewster and other physicists and mineralogists and it only remained to apply their methods to the minerals visible in rock sections.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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