Estimates of the in-water spectral scalar irradiance, E-0, are needed
to quantify the photosynthetically available radiation. When a highly
scattering, optically thick medium is illuminated at its surface, it i
s possible under certain conditions for E-0 to increase with penetrati
on depth near the surface, even if there are no internal sources at th
e wavelength of interest. Analysis and numerical examples presented he
re help to explain and quantify the magnitude and location of potentia
l subsurface E-0 peaks in source-free ocean waters and the dependence
of the phenomenon on the seawater optical properties and surface condi
tions. Peaking in E-0 most likely occurs when the incident illuminatio
n is strongly directed at the zenith angle, and the location of the ma
ximum is deepest when the asymmetry of the scattering phase function i
s large. The presence of surface waves and internal reflection greatly
reduces the chance of E-0 peaks being present, making a maximum in E-
0 below the surface possible only if the single scattering albedo, ome
ga(0), is >0.95 in homogeneous waters or at potentially smaller values
if omega(0) increases with depth.