Two spatial patterns of precipitation appear in accordance with the oscillation of zonal mean zonal wind in the troposphere. One precipitation pattern is a squall-line (SL) type, which appears during a limited period when the near-surface wind is strong, and the other is a back-building (BB) type during the rest of the period. For the SL type, a new precipitation system emerges at the front side of a propagating system. On the other hand, a new system emerges at the rear side for the BB type. These precipitation patterns have good coincidence with space-time variation of the vertical flux of horizontal momentum (Fz); Fz becomes large in the stratosphere for the BB type whereas it becomes large in the troposphere for the SL type.
Fz and its convergence are objectively separated into the upward-propagating, stationary, and downward-propagating contributions using a linear group velocity criterion (c.f., Shaw and Lane, 2013). In the stratosphere, the oscillation in the zonal-mean zonal wind is almost maintained by the Fz convergence near the critical level and the convergence is induced by gravity waves propagating from the troposphere. In the troposphere, strong signals of stationary and downward-propagating contributions coexist. It is difficult to perfectly separate them, because slantwise moist convections and gravity waves coexist in the domain at the same time. However, downward-propagating contribution has a dominant role in the acceleration in the troposphere. The method introduced here, therefore, is useful to evaluate the time variations of the relative importance of each contribution. The results also show the importance of the dynamical coupling between the stratosphere and the troposphere through the modulation of precipitation patterns associated with the oscillation of the zonal mean zonal wind.