Under seasonal forcing, eddies spin up in a short time scale (~ 10 days) in the mid-fall and slowly spin down in the late spring. In spite of the strong seasonality of eddy activity, as observed in the real atmosphere, the PV gradient is still robust. Factors affecting the eddy spin-up, spin-down time scales and the interpretation of the robust PV structure are studied. We also find that eddies are saturated and maintain a robust zonal-mean flow thermal structure in the winter season only when the external forcing is strong and varied slowly. Otherwise, the eddy activity is weak and varies almost proportionally with the variation of the external forcing. Whether the theories obtained in the previous equilibration study still hold in spite of the variation of the external forcing is also discussed in this study.
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