We investigate the influence of the curvature of the Earth on a propos
ed atmospheric-correction scheme for the Sea-Viewing Wide-Field-of-Vie
w Sensor (SeaWiFS) by simulating the radiance exiting the top of a sph
erical-shell atmosphere and inserting the result into the proposed cor
rection algorithm. The error in the derived water-leaving reflectance
suggests that the effects of the curvature are negligible for solar ze
nith angles (theta0) less-than-or-equal-to 70-degrees. Furthermore, fo
r theta0 > 70-degrees the error in atmospheric correction can ususally
be reduced if the molecular-scattering component of the top of the at
mosphere reflectance (rho(r)) is computed with a spherical-shell atmos
phere radiative transfer code. Also, for theta0 > 70-degrees the error
in atmospheric correction in a spherical-shell atmosphere, when rho(r
) is computed with a spherical-shell model, can be predicted reasonabl
y well from computations made with plane-parallel atmosphere radiative
transfer codes. This implies that studies aimed at improving atmosphe
ric correction can be made assuming plane-parallel geometry and that t
he investigator can be confident when theta0 > 70-degrees that any imp
rovements will still be valid for a spherical-shell atmosphere as long
as rho(r) is computed in spherical-shell geometry. Finally, a scheme
for computing rho(r) in a spherical-shell atmosphere in a relatively s
imple manner is developed.