Meridional flow in the Sun's convection zone is a single cell in each hemisphere (1 of 4) (IMAGE)

American Association for the Advancement of Science (AAAS)

Meridional flow in the Sun's convection zone is a single cell in each hemisphere (1 of 4)

Caption

Ionized gas inside the Sun moves toward the poles near the surface and toward the equator at the base of the convection zone (at a depth of 200 thousand kilometers or 125 thousand miles). This material relates to a paper that appeared in the 26 June issue of Science, published by AAAS. The paper, by L. Gizon at Max-Planck-Institut für Sonnensystemforschung in Göttingen, Germany and colleagues was titled, "Meridional flow in the Sun's convection zone is a single cell in each hemisphere."

Credit

MPS (Z.-C. Liang)

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