To detect wind field in the upper atmosphere passive methods was used with imaging interferometer technique the main source is O(Ⅰ

Ⅱ) forbidden aurora. For stronger forbidden transition line

two necessary conditions of theoretical calculation are metastable and enough small electron density. O (Ⅰ

Ⅱ) satisfies the conditions and its forbidden lines are indicated. Then the corresponding photochemical reaction of O (Ⅰ

Ⅱ) forbidden aurora was investigated. The conclusion is that 10 forbidden (allowed) lines (557.7 nm

630.0/636.4/639.3 nm

672.8 nm

732.2/733.2 nm

777.7/777.6/777.4 nm) can be used to detect upper atmospheric wind field

5 lines (639.3 nm

672.8 nm

777.7/777.6/777.4 nm) increased comparing to WINDII

the visible wavelengths aurora is enlarged for imaging interferometer.