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- Author or Editor: Takio Muralami x
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Abstract
In the present study a stationary heat source is prescribed to be maximum at 20° latitude, oscillating in time with a period of 15 days and zonal wavenumber 1. The basic equations for excited perturbation waves are the linearized primitive equations in spherical coordinates with a log-pressure system in the vertical. The zonal mean primitive equations are used to predict the time evolution of the mean fields. The numerical integration is done as a marching problem with respect to time for the period from 0 to 30 days.
The prescribed heat source excites eastward and downward propagating Kelvin waves in the equatorial stratosphere. The Kelvin mode is a maximum neat 25 km and damps out rapidly above that level. This, in turn, leads to the decay of the upward westerly momentum flux with height, and to a consequent acceleration of the zonal mean westerly wind near 25 km above the equator. The westerly acceleration amounts to about 2 m sec−1 per month.
Abstract
In the present study a stationary heat source is prescribed to be maximum at 20° latitude, oscillating in time with a period of 15 days and zonal wavenumber 1. The basic equations for excited perturbation waves are the linearized primitive equations in spherical coordinates with a log-pressure system in the vertical. The zonal mean primitive equations are used to predict the time evolution of the mean fields. The numerical integration is done as a marching problem with respect to time for the period from 0 to 30 days.
The prescribed heat source excites eastward and downward propagating Kelvin waves in the equatorial stratosphere. The Kelvin mode is a maximum neat 25 km and damps out rapidly above that level. This, in turn, leads to the decay of the upward westerly momentum flux with height, and to a consequent acceleration of the zonal mean westerly wind near 25 km above the equator. The westerly acceleration amounts to about 2 m sec−1 per month.
