Abstract
With the development of local helioseismology, such as the time-distance technique, investigation of meridional flow and differential rotation in the solar convection zone has become possible. I summarize recent observational results, and review theoretical considerations of meridional circulation in relation to differential rotation, which is now well unveiled in the solar convection zone by helioseismology. © 2007 WILEY-VCH Verlag GmbH & Co. KGaA.
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Shibahashi, H. (2007). Meridional circulation and differential rotation in the solar convection zone. Astronomische Nachrichten, 328(3–4), 264–268. https://doi.org/10.1002/asna.200610728
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