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The influence of the angular velocity distribution on the energy transport in the Sun's convection zone

  • The Sun:Structure Oscillations, Magnetic Cycle, Surface Variations
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Abstract

This contribution is a purely exploratory search to investigate the way the distribution of angular velocity inside the Sun's convection zone affects the energy transport. This is related with problems concerning the magnetic activity, whose appearance at the Sun's surface depends on the shape of the isorotation surfaces, and the latitudinal variations in flux. The proposed model is non-linear and axisymmetric.

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References

  • Belvedere, G. and Paternò, L.: 1976, Solar Phys. 47, 525.

    Google Scholar 

  • Belvedere, G. and Paternò, L.: 1977a, Solar Phys. 52, 191.

    Google Scholar 

  • Belvedere, G. and Paternò, L.: 1977b, Solar Phys. 54, 289.

    Google Scholar 

  • Belvedere, G., Paternò, L., and Stix, M.: 1980a, Geophys. Astrophys. Fluid Dynamics 14, 209.

    Google Scholar 

  • Belvedere, G., Paternò, L., and Stix, M.: 1980b, Astron. Astrophys. 86, 40.

    Google Scholar 

  • Durney, B. R.: 1976, Astrophys. J. 204, 589.

    Google Scholar 

  • Durney, B. R.: 1980, Astrophys. J., in press.

  • Durney, B. R. and Spruit, H. C.: 1979, Astrophys. J. 234, 1067.

    Google Scholar 

  • Gilman, P. A.: 1977, Geophys. Astrophys. Fluid Dynamics 8, 93.

    Google Scholar 

  • Gilman, P. A.: 1978a, Geophys. Astrophys. Fluid Dynamics 11, 157.

    Google Scholar 

  • Gilman, P. A.: 1978b, Geophys. Astrophys. Fluid Dynamics 11, 181.

    Google Scholar 

  • Gilman, P. A. and Glatzmaier, G. A.: 1980, Astrophys. J., submitted.

  • Glatzmaier, G. A. and Gilman, P. A.: 1980a, Astrophys. J., submitted.

  • Glatzmaier, G. A. and Gilman, P. A.: 1980b, Astrophys. J., submitted.

  • Howard, R.: 1979, Astrophys. J. 228, L45.

    Google Scholar 

  • Howard, R.: 1980, private communication.

  • Howard, R. and Harvey, J.: 1970, Solar Phys. 12, 23.

    Google Scholar 

  • Stix, M.: 1976, Astron. Astrophys. 47, 243.

    Google Scholar 

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Authors and Affiliations

  1. Istituto di Astronomia dell' Università di Catania, Italy

    G. Belvedere

  2. Osservatorio Astrofisico di Catania, Italy

    G. La Rosa

  3. Osservatorio Astrofisico di Catania, Italy

    L. Paternò

  4. Istituto di Fisica della Facoltà di Ingegneria dell' Università di Catania, Italy

    L. Paternò

Authors
  1. G. Belvedere
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  2. G. La Rosa
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  3. L. Paternò
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Additional information

Proceedings of the 14th ESLAB Symposium on Physics of Solar Variations, 16–19 September 1980, Scheveningen, The Netherlands.

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Belvedere, G., La Rosa, G. & Paternò, L. The influence of the angular velocity distribution on the energy transport in the Sun's convection zone. Sol Phys 74, 107–110 (1981). https://doi.org/10.1007/BF00151279

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