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U.S. Department of Energy
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High-altitude non-equilibrium infrared emission models. Final report 11 Jun 86-30 Nov 90

Technical Report ·
OSTI ID:5730929
This report describes the development and implementation of models for predicting infrared emission in non-LTE regions of the Earth's atmosphere. Such models are used to stimulate particular atmospheric conditions, both quiescent and aurorally-distributed, in order to extract information from infrared radiance data sets and study the roles of different basic physical processes affecting the upper atmosphere. Specifically, developed is the first line-by-line radiative excitation model for the upper atmosphere, RAD, applied it to the calculation of populations of infrared-active states of CO{sub 2} and CO, simulated the conditions of the SPIRE experiments, and elucidated the role of atomic oxygen in exciting the CO{sub 2} bending modes. Auroral emissions are modeled and the Field Widened Interferometer data set analyzed using a method of spectral decomposition, and NO band heads identified in the lower-thermosphere emissions. Described are the mathematical procedures underlying the model, especially the RAD model, and the physical process incorporated in them.Results are presented from running the models.
Research Organization:
Arcon Corp., Waltham, MA (USA)
OSTI ID:
5730929
Report Number(s):
AD-A-232503/3/XAB; CNN: F19628-86-C-0118
Country of Publication:
United States
Language:
English