Abstract

The status of observations and current theories of spacecraft‐induced optical emission (ram glow) from the Atmospheric Explorer‐C satellite to the most recent shuttle missions is reviewed. To resolve the discrepancy between the observed spectral continuum and the most likely gas‐phase emitter, the NO2 continuum, a second continuum is proposed, lying further to the red and due to true surface emission (chemiluminescence) as a consequence of atomic and molecular oxygen adsorption. An altitude variation modelled on the basis of this mechanism, using laboratory data, offers good agreement with observations by the AE‐E satellite, and is capable of producing the quantitative intensities in general.

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