On the Relationships between Low-Frequency Variations of Earth's
Rotation and Equatorial Atmospheric Angular Momentum
Abstract
This work mainly concerns low-frequency variations of Atmospheric
Angular Momentum (AAM), emphasizing the role of the equatorial region
and its relationships with the length of day LOD, whose observed
time series indicate an accelerating Earth’s rotation over the last
several decades. We applied bivariate and trivariate Empirical Mode
Decomposition methods to extract coherent nonstationary signals from the
monthly time series of $LOD$ and the two components of AAM, i.e., the
mass term MΩ and the motion term
Mr. It is found that, over the global domain, a
decreasing trend of LOD during the last five decades correlates
with an increasing trend in MΩ, whereas the trend
in Mr is negligible. However, there is a
significantly positive trend in Mr of the
equatorial lower troposphere (1000 to 700 hPa), which can be associated
with a larger transfer of eastward momentum due to the accelerating
Earth. Further analyses of spatio-temporal distribution of
Mr anomalies suggest that, at multidecadal time
scales, residual changes in the motion term of AAM across the globe tend
to be in balance. The long-term positive trend in
MΩ, which is dominant over the equatorial
latitude belt, is most likely attributed to prolonged effects of the
global increase in surface pressure from the mid-1970s until the 1990s.
Low-frequency variations of LOD are also found to have a high
correlation with the Atlantic Meridional Oscillation index. Our results
suggest that long-term changes in the Earth’s rotation rate are
partially attributable to the atmospheric and oceanic variability of
comparable time scales.