Geophysical Research Letters
Resolved spectra have been obtained fromth eg rounodf the0 2(a•Age)m issiofnrso m the upper atmosphere utilizing a wide-field interferometer with a cryogenically cooled germaniwn detector. Thc rotational structure of both the (0,0) band at 1.27 vm and the (0,1) band at 1.58 vm are clearly separable from the hydroxyl airglow.T hed ecarya ts of the0 2(a•Agd
Baker, Doran; Steed, Allan; Huppi, Ronald; and Baker, Kay, "Twilight Transition Spectra of Atmospheric O2 IR Emissions" (1975). Space Dynamics Lab Publications. Paper 6.