For a nonzero zonal wavenumber , stationarity requires
A real propagating solution therefore requires a westerly . For there are two meridional wavenumbers:
The source's assertion of two stationary solutions needs these qualifications: at they coincide, and at there is no real meridionally propagating solution. For example gives . Modes with are a separate zonally invariant degeneracy and do not have a defined zonal phase velocity.
Adding to the zonal group velocity and imposing stationarity gives
Thus a localized midlatitude disturbance radiates stationary Rossby wave activity downstream, along one poleward and one equatorward branch. For in the Northern Hemisphere, gives the northeastward branch and the southeastward branch. With strictly constant , these wave rays are straight. Changing latitude cannot bend them within that constant-coefficient model.
To discuss a planet, extend it locally to slowly varying and possibly . The conserved zonal wavenumber in a locally zonally uniform medium then has
For constant and northward propagation in the Northern Hemisphere, decreasing reduces until : the wave ray becomes zonal at a turning latitude and can refract equatorward. The equatorward branch initially encounters larger allowed and becomes more meridional. This local midlatitude description eventually needs replacement near the equator or wherever the background varies rapidly.
Orographic forcing by a mountain range or persistent spatially localized heating can supply such a disturbance. Its steady forcing selects the ground-stationary part of the response. The corresponding local total wavelength is
For fixed it increases toward the pole as decreases. Locally the zonal integer scale has upper bound , so fewer planetary-scale zonal waves fit around higher-latitude circles. This is not an unconditional trend in actual weather: changing , its curvature, stratification and the forcing spectrum can change the dominant Rossby wave wavelengths.