Detailed knowledge of the molecular spectra of ozone and other infrared-active atmospheric species is needed for accurate calculation of atmospheric heating and cooling rates in climate models. Remote sensing experiments on the Nimbus-7 satellites and the Spacelab-3 Space Shuttle Mission have shown that space-based measurements of infrared absorption or emission can be used to accurately determine the concentrations and distributions of stratospheric species on a global scale. The objective of this research task is to improve knowledge of the spectroscopic line parameters (positions, intensities, assignments, halfwidths, and pressure-induced shifts) of key atmospheric constituents through laboratory measurements.
High resolution spectroscopy to support atmospheric measurements
1990-01-01
Miscellaneous
No indication
English
FTIR Spectroscopy for Atmospheric Measurements
NTRS | 1996
|Atmospheric Wind Measurements with the High-Resolution Doppler Imager
Online Contents | 1995
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