Abstract

Spectral irradiances (0.25–2.5 μ) of individual inert gases and combinations of inert gases have been obtained under a variety of experimental conditions. It has been found that certain experimental parameters influence the spectral distribution more than others, and certain mixture ratios lead to improved solar simulation.

© 1970 Optical Society of America

Vacuum Ultraviolet Plasma Arc Radiation Source for the 300–1000-A Wavelength Region

M. E. Levy and R. E. Huffman
Appl. Opt. 9(1) 41-47 (1970)

Solar Simulators at the Jet Propulsion Laboratory

R. E. Bartera, H. N. Riise, and C. G. Miller
Appl. Opt. 9(5) 1068-1074 (1970)

Solar Spectral Irradiance Measured from 11.58 km with a Leiss Monochromator and a Photoelectric Filter Radiometer

J. J. Webb, C. H. Duncan, R. McIntosh, and D. Lester
Appl. Opt. 9(2) 345-349 (1970)

Spectral Radiance Between 0.42 μ and 1.1 μ of Rubidium and Cesium Vapor Arc Lamps as Function of Power Input and Pressure

D. Fromm
Appl. Opt. 9(4) 913-923 (1970)

Ultraviolet Emission Spectra of High-Pressure Rare Gases

Philip M. Johnson
J. Opt. Soc. Am. 60(12) 1669-1674 (1970)