Atomic Emission in Th• Ultraviolet Nightglow
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چکیده
An observation of the ultraviolet nightglow between 2670/• and 3040/• was conducted over White Sands Missile Range on October 22, 1984, at 0020 hours LST during the Orionids meteor shower. A 1/4-meter uv spectrometer operating at 3.5/• resolution viewed the Earth's limb at tangent heights between 90 km and 110 km for 120 seconds. By inverting the observed limb intensities, a total zenith intensity of 1.4 kR is inferred for the HerzbergoI system. Excess emission above the Hemberg I (7,3) band at 2852 A is identified as the Mg I resonance line. The intensity ratio of the Hemberg I band system to the 2972/• line from O(1 S) was less than that predicted from the accepted O(1 S) b. ranching ratio and acceptable ratios of Herzberg I to 5577A emissions. Arguments supporting the identification of the Herzberg III band system are also advanced.
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تاریخ انتشار 2007