“…Photodecomposition rates in air for a number of aldehydes and ketones are calculated from the actinic fluxes within the planetary boundary layer (Dimerjian et al, 1980), along with absorption cross-sections and quantum yields, ~z (F6rgeteg et al, 1979;Horowitz and Calvert, 1982;Gardner et aL, 1984;Desai et aL, 1989;Heicklen et al, 1986;Meyrahn et al;Atkinson et al, 1986), or from photolysis rates relative to NO 2 (Plum et aL, 1983). For CH3COC2Hs, a 9~a of 0.1 is assumed (Carter et al, 1986), and for C2HsCOC2H 5 and (CH3)2CHCOCH 3, a #z of 0.2 is assumed within the range of 295 um to 340 nm.…”