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LASER ACTION UP TO 57.355 μ IN GASEOUS DISCHARGES (Ne, He–Ne)
1.W. L. Faust, R. A. McFarlane, C. K. N. Patel, and C. G. B. Garrett, “New Infrared Maser Lines of the Noble Gases,” Bull. Am. Phys. Soc. 8, 299 (April, 1963).
2.W. L. Faust, R. A. McFarlane, C. K. N. Patel, and C. G. B. Garrett, “Noble Gas Optical Maser Lines at Wavelengths Between 2 μ and 35 μ,” Phys. Rev. (to be published).
3.The general features of maser setups for investigation in the far infrared have been described in detail in ref 2.
4.F. J. Low, “Low Temperature Germanium Bolometer,” J. Opt. Soc. Am. 51, 1300–1304 (November, 1961).
5.P. L. Richards (unpublished work).
6.G. D. Boyd and J. P. Gordon, “Confocal Multimode Resonator for Millimeter Through Optical Wavelength Masers,” Bell System Tech. J. XL, 489–509 (March, 1961).
7.W. L. Faust and R. A. McFarlane, “Line Strengths for Noble Gas Maser Transitions; Calculations of Gain/Inversion at Various Wavelengths,” J. Appl. Phys. (to be published).
8.C. E. Moore, Atomic Energy Levels, National Bureau of Standards Circular 467 (U.S. Government Printing Office, Washington, D.C.).
9.R. A. McFarlane, Bull. Am. Phys. Soc., Ser. II 8, 359 (1963).
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