that we can solve rapidly to obtain J\ as a function of optical depth for each wavelength, given the boundary conditions at the top of the atmosphere and at the surface. The upwards and downwards diffuse spectral fluxes at each atmospheric level can then be calculated from

so that the net downwards diffusive flux is 4nHX, while the total flux available l°Fd X, for photolysis is 4nJX + MqFJ-, , so that the enhancement factor for photolysis is

posq x

H can be computed from

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