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<p><strong>Abstract.</strong> Relative vibrational populations of triplet <I>B</I><sup>3</sup>&Pi;<sub><I>g</I></sub>, <I>W</I><sup>3</sup>&Delta;,sub><I>u</I></sub>, <I>B</I><sup>'3</sup>&Sigma;<sub><I>u</I></sub><sup>&minus;</sup> states of N<sub>2</sub> and the <I>b</I><sup>1</sup>&Sigma;<sub><I>g</I></sub><sup>+</sup> state of O<sub>2</sub> are calculated for different altitudes of the high-latitude upper atmosphere during auroral electron precipitation. It is shown thatdoi:10.5194/angeo-26-1159-2008 fatcat:44pi4eifcnajzavookgdesonhu