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Origin of the Sun's Differential Rotation

Published online by Cambridge University Press:  08 February 2017

L.L. Kichatinov
L.L. Kichatinov*
Affiliation:
Siberian Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation (SibIZMIR) 664697 Irkutsk, P.O. Box 4 USSR

Abstract

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The present status of the Sun's differential rotation theories is reviewed. Attention is mainly focused on mechanisms for differential rotation based on the anisotropic viscosity concept and their modern developments within the framework of the mean-field hydrodynamics. The models with latitude-dependent heat transport and non-axisymmetric numerical simulations are briefly discussed.

Type
V. Large-scale Structure and Dynamics
Information
Symposium - International Astronomical Union , Volume 138: Solar Photosphere: Structure, Convection and Magnetic Fields , 1990 , pp. 297 - 307
Copyright
Copyright © Kluwer 1990 

References

REFERENCES

Altrock, R.C. and Canfield, R.C. (1972) Sol. Phys. 23, 343–354.Google Scholar
Baker, N. and Temesvary, S. (1966) Tables of Convective Stellar Envelope Models, 2nd ed. Goddard Institute for Space Studies, New York.Google Scholar
Belvedere, G. and Paterno, L. (1977) Sol. Phys. 54, 289–312.Google Scholar
Belvedere, G., Paterno, L. and Stix, M. (1980 Geophys. Astrophys. Fluid Dynamics 14, 209–224.CrossRefGoogle Scholar
Bierman, L. (1951) Z. Astrophysic 28, 304.Google Scholar
Brown, T.M. (1985) Nature 317, 591–594.CrossRefGoogle Scholar
Brown, T.M. and Morrow, C.A. (1987) Astrophys J. 314, L21–L26.Google Scholar
Carrington, R.C. (1863) Observations of the Spots on the Sun, Williams & Norgate, London.Google Scholar
Cocke, W.J. (1967) Astrophys. J. 150, 1041–1050.Google Scholar
Deubner, F.-L., Ulrich, R.K. and Rhodes, E.J. (1979) Astron. Astrophys. 72, 177–185.Google Scholar
Durney, B.R. and Roxburg, I.W. (1971) Sol. Phys. 16, 3–20.Google Scholar
Durney, B.R. and Spruit, H.C. (1979) Astrophys. J. 234, 1067.CrossRefGoogle Scholar
Durney, B.R. and Latour, J. (1978) Geophys. Astrophys. Fluid Dynamics 9, 241–255.Google Scholar
Duvall, T.L. (1979) Sol. Phys. 63, 3–15.CrossRefGoogle Scholar
Duvall, T.L., Dziembowski, W.A., Goode, P.R., Gough, D.O., Harvey, J.W. and Leibacher, J.W. (1984) Nature 310, 22–25.CrossRefGoogle Scholar
Duvall, T.L., Harvey, J.W. and Pomerantz, M.A. (1986) Nature 321, 500–501.Google Scholar
Falciani, R., Rigutti, M. and Roberti, G. (1974) Sol. Phys. 35, 277–280.Google Scholar
Gilman, P.A. (1980) Lecture Notes in Phys. 114, 19–37.Google Scholar
Gilman, P.A. and Glatzmaier, G.A. (1981) Astrophys. J. Suppl. 45, 335–349.Google Scholar
Gilman, P.A. and Howard, R. (1984) Sol. Phys. 93, 171–175.Google Scholar
Gilman, P.A. and Miller, J. (1986) Astrophys. J. Suppl. 61, 585.Google Scholar
Glatzmaier, G.A. (1984) J. Comput. Phys. 55, 461–484.Google Scholar
Glatzmaier, G.A. (1985a) Astrophys. J. 291, 300–307.Google Scholar
Glatzmaier, G.A. (1985b) Geophys. Astrophys. Fluid Dyn. 31, 137.CrossRefGoogle Scholar
Gough, D.O. (1969) J. Atmosph. Sci. 26, 448–456.2.0.CO;2>CrossRefGoogle Scholar
Gough, D.O. and Weiss, N.O. (1976) Mon. Not. Roy. Astr. Soc. 176, 589–607.CrossRefGoogle Scholar
Howard, R. (1984) Ann. Rev. Astron. Astrophys. 22, 131–155.Google Scholar
Howard, R. and Harvey, J. (1970) Sol. Phys. 12, 23–51.Google Scholar
Iroshnikov, R.S. (1969) Astron. J. (SSSR) 46, 97–112.Google Scholar
Kichatinov, L.L. (1986) Geophys. Astrophys. Fluid Dyn. 35, 93.Google Scholar
Kichatinov, L.L. (1987) Geophys. Astrophys. Fluid Dyn. 38, 273.CrossRefGoogle Scholar
Kichatinov, L.L.(1988) Astron. Nachr. 309, 197–211.Google Scholar
Kippenhahn, R. (1963) Astrophys. J. 314, 664–678.Google Scholar
Köhler, H. (1970) Sol. Phys. 13, 3–18.Google Scholar
LaBonte, B.J. and Howard, R. (1982) Sol. Phys. 80, 361–372.CrossRefGoogle Scholar
Lebedinski, A.I. (1941) Astron. Zh. 18, 10–25.Google Scholar
Moss, D. and Vilhu, O. (1983) Astron. Astrophys. 119, 47–53.Google Scholar
Noyes, R.W., Ayres, T.R. and Hall, D.N. (1973) Sol. Phys. 28, 343.Google Scholar
Ogura, Y. and Phillips, N.A. (1962) J. Atmosph. Sci. 19, 173.Google Scholar
Pidatella, R.M., Stix, M., Belvedere, G. and Paterno, L. (1986) Astron Astrophys. 156, 22–32.Google Scholar
Rüdiger, G. (1977) Sol. Phys. 51, 257–268.Google Scholar
Rüdiger, G. (1982a) Geophys. Astrophys. Fluid Dyn. 21, 1–25.Google Scholar
Rüdiger, G. (1982b) Astron. Nachr. 303, 293–303.Google Scholar
Rüdiger, G. (1983) Geophys. Astrophys. Fluid Dyn. 25, 213–233.Google Scholar
Rüdiger, G. (1989) Differential Rotation and Stellar Convection, Akademie - Verlag, Berlin.Google Scholar
Sakurai, T. (1966) Publ. Astron. Soc. Japan 18, 174–200.Google Scholar
Schmidt, W. (1982) Geophys. Astrophys. Fluid Dyn. 21, 27–57.Google Scholar
Schröter, E.H. (1985) Sol. Phys. 100, 141–169.CrossRefGoogle Scholar
Spruit, H.C. (1974) Sol. Phys. 34, 277–290.Google Scholar
Tayler, R.J. (1973) Mon. Not. Roy. Astron. Soc 165, 39–52.CrossRefGoogle Scholar
Tuominen, J., Tuominen, I. and Kyröläinen, J. (1983) Mon. Not. Roy. Astron. Soc. 205, 691–702.Google Scholar
Vandakurov, Yu. V. (1982) Astrophys. Space Sci. 83, 105–116.Google Scholar
Ward, F. (1965) Astrophys. J. 141, 534–547.Google Scholar
Wasiutinski, J. (1946) Astrophys. Norvegica 4, 1.Google Scholar
Weiss, N.O. (1965) Observatory 85, 37–39.Google Scholar