Abstract
A minimum of angular velocity is not found at the equator as suggested by Gilman, but at a latitude of 6° in both hemispheres.
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References
Deubner, F. -L. and Liedler, R.: 1969, Solar Phys. 7, 87.
Gilman, P. A.: 1972, Solar Phys. 27, 3.
Howard, R. and Harvey, J.: 1970, Solar Phys. 12, 23.
Newton, H. W. and Nunn, M. L.: 1951, Monthly Notices Roy. Astron. Soc. 111, 143.
Solonsky, Y. A.: 1972, Solar Phys. 23, 3.
Wilcox, J. M. and Howard, R.: 1970, Solar Phys. 13, 251.
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Mitteilung aus dem Fraunhofer-Institut, No. 136.
On leave from Institute Universitario de Astrofisica, Universidad de La Laguna, Tenerife, Spain.
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Deubner, FL., Vazquez, M. Differential rotation and the spot zones. Sol Phys 43, 87–90 (1975). https://doi.org/10.1007/BF00155145
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DOI: https://doi.org/10.1007/BF00155145