Atmospheric radical production by excitation of vibrational overtones via absorption of visible light

We present calculations using a radiative transfer model which predict that in the lower stratosphere at high zenith angles, significant enhancements to the photodissociation rates of HNO 3 and HNO 4 can result from visible wavelength excitation of OH overtone vibrations containing sufficient energy to cleave the O‐O and N‐O bonds. The results indicate that atmospheric chromophores such as HONO 2 , HO 2 NO 2 and H 2 O 2 , could make a potentially significant contribution to the production of HO x and NO x . Calculating the relative importance of their effect requires better knowledge of the absolute absorption cross sections, both for vibrational overtones and in the near UV. Stratospheric air masses in which this process could be important are those that experience lengthy exposure at high solar zenith angles: the outer regions of the polar winter vortex and the polar summer anticyclone. We note that the general mechanism may have application elsewhere, such as in the atmospheres of other planets and in generating the diffuse interstellar bands associated with molecular clouds.