Authors: Sushant S. Mahajan (W. W. Hansen Experimental Physics Laboratory, Stanford University), Xudong Sun (Institute for Astronomy, University of Hawaii), Junwei Zhao (W. W. Hansen Experimental Physics Laboratory, Stanford University)

Using time-distance local helioseismology flow maps within 1 Mm of the solar photosphere, we detect inflows toward activity belts that contribute to solar cycle scale variations in near-surface meridional flow. These inflows stretch out as far as 30 degrees away from active region centroids. If active region neighborhoods are excluded, the solar cycle scale variation in background meridional flow diminishes to below 1~m~s$^{-1}$, but still shows systematic variations in the absence of active regions between sunspot cycles 24 and 25. We, therefore, propose that the near-surface meridional flow is a three component flow made up of: a constant baseline flow profile that can be derived from quiet Sun regions, variations due to inflows around active regions, and solar cycle scale variation of the order of $<$ 1~m~s$^{-1}$. Torsional oscillation, on the other hand, is found to be a global phenomena i.e. exclusion of active region neighborhoods does not affect its magnitude or phase significantly. This non-variation of torsional oscillation with distance away from active regions and the three-component breakdown of the near-surface meridional flow serve as vital inputs for solar dynamo models and surface flux transport simulations.