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A calculation of the fluorescent scattering spectrum of the solar Lyman alpha line by the (14, 0)band of the CO 4(+) system is presented. It is shown that emissions from the υ′ = 14 level of the A¹Π state dominate the total scattering spectrum at column densities of 1018 molecules/cm² and at ambient temperatures.
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Thomas Kassal (1976) studied this question.
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