Absolute Solar Spectra 35–55 Microns II Theoretical Spectra for Altitude Range 15–30 km
- 1 April 1964
- journal article
- Published by Optica Publishing Group in Applied Optics
- Vol. 3 (4) , 459-465
- https://doi.org/10.1364/ao.3.000459
Abstract
Transmission functions are applied to a model representing the atmosphere for specified pressures and concentrations of absorbing gases corresponding to total atmospheric paths above altitudes of 15 km to 30 km and zenith angles of 0° and 40°. The computed transmittance is then applied to the solar spectral radiance envelope curve obtained in Part I to give solar spectra with 0.02-μ resolution in the range 3.5–5.5 μ.Keywords
This publication has 9 references indexed in Scilit:
- Absolute Solar Spectra 35–55 Microns I Experimental Spectra for Altitude Range 0–15 kmApplied Optics, 1964
- Useful representations for measurements of spectral band absorptionJournal of the Optical Society of America, 1960
- Pressure Modulation of Infrared Absorption* I Entire Vibration-Rotation BandsJournal of the Optical Society of America, 1958
- Models for Spectral Band Absorption*Journal of the Optical Society of America, 1958
- Atmospheric Transmission in the InfraredJournal of the Optical Society of America, 1957
- A statistical model for water‐vapour absorptionQuarterly Journal of the Royal Meteorological Society, 1952
- A Grating Map of the Solar Spectrum from 3.0 to 5.2 Microns.The Astrophysical Journal, 1951
- Carbon Dioxide Content of Atmospheric AirNature, 1944
- Mean Absorption and Equivalent Absorption Coefficient of a Band SpectrumPhysical Review B, 1938