Abstract

Solar spectra in the region of the 4.75-μ ozone band have been obtained on a new high-resolution grating spectrometer. By comparing the solar spectrum with a laboratory spectrum of this O₃ band, almost 300 O₃ lines have been identified in the solar spectrum. This region of the solar spectrum also contains lines of H₂O, CO, and CO₂, which greatly perturb the appearance of the O₃ band in the solar spectrum.

© 1963 Optical Society of America

The 15–26 Micron Sky Emission Spectrum at Jungfraujoch (3570 m)

H. J. Bolle
Appl. Opt. 2(6) 571-580 (1963)

Infrared Transmission of the Atmosphere to Solar Radiation

David M. Gates and Walter J. Harrop
Appl. Opt. 2(9) 887-898 (1963)

Computed Transmission Spectra for 27-Micron H₂O Band

David M. Gates, Robert F. Calfee, and David W. Hansen
Appl. Opt. 2(11) 1117-1122 (1963)

Long Path Atmospheric Ozone Absorption in the 9–10-μ Region Observed from a Balloon-Borne Spectrometer

A. Goldman, T. G. Kyle, D. G. Murcray, F. H. Murcray, and W. J. Williams
Appl. Opt. 9(3) 565-580 (1970)

Variation of the Infrared Solar Spectrum Between 700 cm⁻¹ and 2240 cm⁻¹ with Altitude

D. G. Murcray, F. H. Murcray, W. J. Williams, T. G. Kyle, and A. Goldman
Appl. Opt. 8(12) 2519-2536 (1969)