It is pointed in this paper that the influence of the component of nongeostrophic windon the potential vorticity transportation in the north-south direction must be considered inthe energy propagations of stationary planetary waves. Then, the wave action conservationequation for planetary waves is demonstrated and the wave action flux, i.e. Eliassen-Palmflux, is obtained in a spherical atmosphere. It is also demonstrated by WKBJ method in this paper that the distribution of E-R fluxvector due to planetary wave is parallel to the local group velocity of waves. Stationary planetary waves responding to an idealized forcing mechanism are computed bymeans of a multi-level model. It is verified by the distributions of E-P flux vector thatthere are two wave guides in the stationary planetary wave propagations in a spherical at-mosphere in winter, i.e. there should be another wave guide pointing from the troposphere atmiddle latitudes toward the upper troposphere at low latitudes in addition to the polar wavegu It is pointed in this paper that the influence of the component of nongeostrophic windon the potential vorticity transportation in the north-south direction must be considered inthe energy propagations of stationary planetary waves. Then, the wave action conservationequation for planetary waves is demonstrated and the wave action flux, ie Eliassen-Palmflux, is obtained in a spherical atmosphere. It is also demonstrated by WKBJ method in this paper that the distribution of ER flux vector due to planetary wave is parallel to the local group velocity of waves. an idealized forcing mechanism are computed bymeans of a multi-level model. It is verified by the distributions of EP flux vector thatthere are two wave guides in the stationary planetary wave propagations in a spherical at-mosphere in winter, ie there should be another wave guide pointing from the troposphere atmiddle latitudes toward the upper troposphere at low latitudes in addition t o the polar wavegu