摘要
The rate coefficients of vibrational excitation of ground-state molecules N2(X1危g+) and O2(X3危g鈭?/sup>) in processes of the quenching of electronically excited molecules N2(A3危u+, B3螤g, W3螖u, 袙鈥?sup>3危u鈭?/sup>, a鈥?sup>1危u鈭?/sup>, a1螤g, w1螖u) and O2(a1螖g, b1危g+, c1危u鈭?/sup>, A鈥?sup>3螖u, A3危u+) 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 X1危g+ 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 A3危u+ and a1螤g states for vibrational levels v鈥?gt;10, intramolecular electron energy transfer process in N2(A3危u+,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 a1螖g, b1危g+, and three Herzberg c1危u鈭?/sup>, A鈥?sup>3螖u, A3危u+ electronically excited states of molecular oxygen through radiational and collisional quenching are important in vibrational excitation of ground-state molecule O2(X3危g鈭?/sup>,v鈥?2-37).