We study analytically and numerically a class of traveling and standing wav
es in a model of weakly non-linear gravity water waves on the sphere. These
waves are 'near-monochromatic' in space, i.e. their amplitude consists of
one spherical harmonic plus small corrections, and we see numerically that
they retain this property for long time. A main feature of the model we con
sider is that it possesses a Hamiltonian structure. This structure is prese
rved by our numerical implementation, and we use formal and rigorous argume
nts from classical perturbation theory to understand the numerical observat
ions. (C)1999 Elsevier Science B.V. All rights reserved.