Solar occultation spectra obtained with a balloon-borne interferometer have been used to study continuous absorption by N 2 and CO 2 near 2400 cm-' in the lower stratosphere. Synthetic continuum transmittances, calculated from published coefficients for far-wing absorption by CO 2 lines and for pressure-induced absorption by the fundamental band of N 2 , are in fair agreement with the observed stratospheric values. The continuum close to the V3 R-branch band head of CO 2 is sensitive to the CO 2 far-wing line shape. Therefore, given highly accurate knowledge of the N 2 continuum from laboratory data, high-resolution stratospheric spectra provide a sensitive means for in situ testing of various air-broadened CO 2 line shapes at low temperatures.