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《New Astronomy Reviews》2002,46(8-10):567-571
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M.H. Rees 《Planetary and Space Science》1984,32(3):373-378
The results of recent laboratory experiments suggest that the reaction N+ + O2 → NO+ + O(1S) is the principal source of O(1S) in aurora. A negligible time delay between auroral ionization and O(1S) production is associated with this indirect process, which is a necessary condition for a viable mechanism. The volume emission rate ratio associated with this production source remains constant with altitude. The problems encountered by the currently accepted source of O(1S), the reaction of N2(A3Σ) molecules with atomic oxygen are explored, and the contributions of this and other reactions to the auroral green line emission are reevaluated. 相似文献
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