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The time dependent optical emission model developed by Liu and Pasko (2004) is applied to studies of far‐UV emissions of sprite streamers due to N 2 Lyman‐Birge‐Hopfield (LBH) band system. Modeling results indicate that the LBH emissions of sprite streamers at 70 km are generally stronger by up to a factor of 10 than those from the first negative band system of N 2 + , and experimental measurements of the ratio of these two emissions at sprite altitudes can be used to determine poorly known quenching altitude of the N 2 ( a 1 Π g ) state.
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Liu et al. (2005) studied this question.
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