Fig. 3

January mean amplitudes of geopotential height variations (gpm) produced by stationary planetary wave modes with zonal wavenumbers 1, 2, 3, and 4 (panels from the top to the bottom, respectively) for the easterly QBO phase without OGW effects a. The amplitudes differ due to involving OGW effects in the easterly QBO phase b and due to change in QBO phase from easterly to westerly without OGW c. Solid contours in panels b and c correspond to zero differences