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Influence of electronically excited N2 and O2 on vibrational kinetics of these molecules in the lower thermosphere and mesosphere during auroral electron precipitation
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摘要
The rate coefficients of vibrational excitation of ground-state molecules N2(X1g+) and O2(X3g鈭?/sup>) in processes of the quenching of electronically excited molecules N2(A3u+, B3g, W3u, 袙鈥?sup>3u鈭?/sup>, a鈥?sup>1u鈭?/sup>, a1g, w1u) and O2(a1g, b1g+, c1u鈭?/sup>, A鈥?sup>3u, A3u+) are calculated according to quantum-chemical approximations. Applying the calculated rate coefficients we have studied the role of inelastic intermolecular and intramolecular electron energy transfer processes in the production of vibrationally excited molecules at altitudes of the lower thermosphere and mesosphere during auroral electron precipitation. The study of vibrational populations (v鈥?2-30) of the X1g+ state of N2 at the altitudes of the lower thermosphere and mesosphere during auroral electron precipitation has shown three principal excitation mechanisms: radiational transitions from the A3u+ and a1g states for vibrational levels v鈥?gt;10, intramolecular electron energy transfer process in N2(A3u+,v=0-5)+N2 collisions for vibrational levels v鈥?25-30 and the excitation by auroral electrons. Calculations have shown that transitions from two singlet a1g, b1g+, and three Herzberg c1u鈭?/sup>, A鈥?sup>3u, A3u+ electronically excited states of molecular oxygen through radiational and collisional quenching are important in vibrational excitation of ground-state molecule O2(X3g鈭?/sup>,v鈥?2-37).

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