GLOBAL ATMOSPHERIC SEASONAL-MEAN HEATING：DIABATIC VERSUS TRANSIENT HEATING

With the ERA40 reanalysis daily data for 1958-2001, the global atmospheric seasonal-mean diabatic heating and transient heating are computed by using the residual diagnosis of the thermodynamic equation. The three-dimensional structures for the two types of heating are described and compared. It is demonstrated that the diabatic heating is basically characterized by strong and deep convective heating in the tropics, shallow heating in the midlatitudes and deep cooling in the subtropics and high-latitudes. The tropical diabatic heating always shifts towards the summer hemisphere, but the midlatitude heating and high-latitude cooling tend to be strong in the winter hemisphere. On the other hand, the transient heating due to transient eddy transfer is characterized by a meridional dipole pattern with cooling in the subtropics and heating in the mid- and high-latitudes, as well as by a vertical dipole pattern in the midlatitudes with cooling at lower levels and heating in the mid- and higher-levels, which gives rise to a sloped structure in the transient heating oriented from the lower levels in the high latitudes and higher levels in the midlatitudes. The transient heating is closely related to a storm track along which the transient eddy activity is much stronger in the winter hemisphere than in the summer hemisphere. In Northern Hemisphere, the transient heating locates in the western oceanic basin, while it is zonally-oriented in Southern Hemisphere, for which the transient heating and cooling are far separated over South Pacific during the cold season. The transient heating tends to cancel the diabatic heating over most of the globe. However, it dominates the mid-tropospheric heating in the midlatitudes. Therefore, the atmospheric transient processes act to help the atmosphere gain more heat in the high-latitudes and in the mid-troposphere of midlatitudes, reallocating the atmospheric heat obtained from the diabatic heating.