Subthermal nitric oxide spin-orbit distributions in the thermosphere

Physics

Scientific paper

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Atmospheric Composition, Atmospheric Radiation, Atoms, Nitric Oxide, Photodissociation, Spatial Distribution, Spectral Emission, Thermosphere, Earth Radiation Budget, Kinetics, Orbits, Remote Sensing, Thermodynamic Equilibrium

Scientific paper

The two NO(X2)pi, upsilon = 1, Omega = 1/2,3/2) spin-orbit populations in the Earth's thermosphere have been found to depart by more than a factor of 2 from the ratio expected from thermal equilibrium. The effective temperature describing the observed population distribution is as much as 700 K lower than the local kinetic temperature. Absolute NO(upsilon = 1, J, Omega) column densities were derived from high-resolution (1/cm) infrared earthlimb spectra for tangent altitudes up to 200 km, obtained in the Cryogenic InfraRed Radiance Instrumentation for Shuttle (CIRRIS) 1A Space Shuttle Experiment. Nonlinear least-squares synthetic spectral fitting was used to analyze the NO delta upsilon = 1 fundamental band emissions near 5.3 micrometers. The spin-orbit distribution represents a third degree of freedom, along with vibration and rotation, that is not in equilibrium with the local kinetic temperature. These observations may significantly impact the interpretation of band-integrated measurements of NO in the upper atmosphere, for which equilibrium sublevel distributions have been assumed. The subthermal distribution is most likely produced in the collisional uppumping of NO(upsilon = 0) by O atoms, which is the major source of NO(upsilon = 1) in the thermosphere. This inference suggests that the present effect is related to the subthermal spin-orbit distributions observed in laboratory studies of NO2 photodissociation.

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