  A key component of solar interior dynamics is the meridional circulation
(MC), whose poleward component in the surface layers has been well observed.
Time-distance helioseismic studies of the deep structure of MC, however, have
yielded conflicting inferences. Here, following a summary of existing results
we show how a large center-to-limb systematics (CLS) in the measured travel
times of acoustic waves affect the inferences through an analysis of frequency
dependence of CLS, using data from the Helioseismic and Doppler Imager (HMI)
onboard Solar Dynamics Observatory (SDO). Our results point to the residual
systematics in travel times as a major cause of differing inferences on the
deep structure of MC.
