Spectra of ozone υ 3 emission in an auroral nighttime sky were obtained in the Spectral Infrared Interferometric Telescope experiment. High‐quality hot band spectra reveal spectral structure not previously observable and provide a critical test of ozone radiance models. The limb radiance profile is in good agreement with previous data below ∼95 km, but above this it falls off more rapidly.
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Adler‐Golden et al. (1990) studied this question.
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