Evolving Submerged Meridional Circulation Cells within the Upper Convection Zone Revealed by Ring‐Diagram Analysis

TLDR

The study reports large‑scale meridional and zonal flows observed from 1996 to 2001. Ring‑diagram analysis of MDI data revealed that the upper‑convection‑zone meridional flow develops additional, latitude‑ and depth‑wandering submerged cells that create hemispheric asymmetry, disrupt poleward flow, and could significantly influence angular‑momentum transport, magnetic‑field dynamics, and the near‑surface rotational shear layer.

Abstract

Using the local helioseismic technique of ring-diagram analysis applied to Michelson Doppler Imager (MDI) Dynamics Program data from the Solar and Heliospheric Observatory, we have discovered that the meridional flow within the upper convection zone can develop additional circulation cells whose boundaries wander in latitude and depth as the solar cycle progresses. We report on the large-scale meridional and zonal flows that we observe from 1996 to 2001. In particular, we discuss the appearance and evolution of a submerged meridional cell during the years 1998-2001, which arose in the northern hemisphere and disrupted the orderly poleward flow and symmetry about the equator that is typically observed. The meridional flows in the southern and northern hemispheres exhibit striking asymmetry during the past four years of the advancing solar cycle. Such asymmetry and additional circulation cells should have profound impact on the transport of angular momentum and magnetic field within the surface layers. These flows may have a significant role in the establishment and maintenance of the near-surface rotational shear layer.