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Models of solar differential rotation
1984o-.rr rcdels give the deperrdence of the angular velocity at the Sunis equator on the depth of the convecÈion zcne. In order to drive differential rotation we ccnsidered two different rnechanisxns: latirude depe:rience of the n:xj"ng length and the anisoircpy of :ie turbulent viscosity.
Pidatella, Rosa Maria +3 more
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Hydrodynamical Investigation of the Solar Differential Rotation
Publications of the Astronomical Society of Japan, 1966Abstract The differential rotation of the sun is investigated from Biermann’s viewpoint which ascribes its cause to the non-isotropy of the eddy viscosity. The hydrogen convection layer is considered to be a thin layer rotating independently of the inner stable region, and its rotational motion is investigated on the basis of Wasiutyński’
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On the differential rotation with height in the solar atmosphere
Solar Physics, 1969Spectroscopic measurements of solar rotation having good height discrimination show no change in angular velocity through the photosphere layers but an increase of 8% for the Hα chromosphere (epoch 1968.9). Spectroscopic results in general are compared with measures made with tracers, i.e.
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Solar differential rotation reproduced with high-resolution simulation
Nature Astronomy, 2021H Hotta, K Kusano, Kusano K
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Characterizing the feedback of magnetic field on the differential rotation of solar-like stars
Advances in Space Research, 2016J Varela, A Strugarek, A S Brun
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Long-Term Variations of Solar Differential Rotation and Sunspot Activity: Revisited
Solar Physics, 2013K J Li, X J Shi, H F Liang
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Differential rotation and sector structure of solar magnetic fields
Solar Physics, 1974J O Stenflo, Stenflo J O
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Investigation of the Solar Differential Rotation of Compact Magnetic Elements for 1966 – 1986
Solar Physics, 2009D R Japaridze
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