The Optical Constants of Crystals of Selenium and Tellurium for Wave-Lengths from 3000 to 5000 Angstroms
- 1 June 1925
- journal article
- Published by Optica Publishing Group in Journal of the Optical Society of America
- Vol. 10 (6) , 621-634
- https://doi.org/10.1364/josa.10.000621
Abstract
The measurements were made by a photographic method, for two positions of the crystal, (1) with the optic axis parallel, and (2) with the axis perpendicular to the plane of incidence. Two sets of optical constants were found for each substance. For selenium, in the parallel position the index of refraction was found to vary from 3.4 to 4.4, and the reflecting power from 0.38 to 0.46; in the perpendicular position the index varies from 2.3 to 3.1, and the reflecting power from 0.41 to 0.34. For tellurium, in the parallel position the index varies from 1.9 to 2.9, and the reflecting power from 0.10 to 0.27; in the perpendicular position the index varies from 1.7 to 2.7, the reflecting power from 0.09 to 0.23. The average error is estimated to be about 5 per cent. The accuracy is greatest for the middle range of wavelengths, 3500-4000 A.Keywords
This publication has 9 references indexed in Scilit:
- Note on the Principal Reflecting Powers of TelluriumJournal of the Optical Society of America, 1923
- On the Optical Constants of Selenium in the form of Isolated CrystalsJournal of the Optical Society of America, 1922
- The CrystelliptometerAn Instrument for the Polariscopic Analysis of Very Slender Beams of LightJournal of the Optical Society of America, 1922
- The Optical Properties of an Isolated Crystal of SeleniumPhysical Review B, 1917
- The Light Sensitiveness of Copper OxidePhysical Review B, 1916
- The Reflecting Power of Metals in the Ultra-Violet Region of the SpectrumThe Astrophysical Journal, 1915
- Untersuchungen über Dispersion und Absorption bei Metallen für das sichtbare und ultraviolette SpektrumAnnalen der Physik, 1910
- Metallic Arcs for Spectroscopic InvestigationsThe Astrophysical Journal, 1908
- Dispersion einiger Metalle, besonders für ultraviolette StrahlungAnnalen der Physik, 1903