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Spatially-resolved Analysis of the Upper Convection Zone

  • R. S. Bogart (a1), J. Schou (a1), S. Basu (a2), D. A. Haber (a3), F. Hill (a4) and H. M. Antia (a5)...

Abstract

Ring-diagram analysis of MDI data has revealed systematic patterns in global flow patterns in the early phase of the cycle. We report on variations and trends seen in the flows in subsequent years.

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References

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Basu, S., Antia, H. M., & Tripathy, S. C. 1998, in ESA SP-418, Structure and Dynamics of the Interior of the Sun and Sun-like Stars, ed. Korzennik, S. & Wilson, A. (Dordrecht: ESA), 705.
Haber, D. A., Hindman, B. W., Toomre, J., Bogart, R. S., Schou, J., & Hill, F. 1998, in ESA SP-418, Structure and Dynamics of the Interior of the Sun and Sun-like Stars, ed. Korzennik, S. & Wilson, A. (Dordrecht: ESA), 791.

Spatially-resolved Analysis of the Upper Convection Zone

  • R. S. Bogart (a1), J. Schou (a1), S. Basu (a2), D. A. Haber (a3), F. Hill (a4) and H. M. Antia (a5)...

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