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Spatially-resolved Analysis of the Upper Convection Zone

Published online by Cambridge University Press:  13 May 2016

R. S. Bogart ,
J. Schou ,
S. Basu ,
D. A. Haber ,
F. Hill  and
H. M. Antia
R. S. Bogart
Affiliation:
Stanford University, CSSA-HEPL, Stanford CA 94305-4085, USA
J. Schou
Affiliation:
Stanford University, CSSA-HEPL, Stanford CA 94305-4085, USA
S. Basu
Affiliation:
Yale University, P.O. Box 208101, New Haven CT 06520-8101, USA
D. A. Haber
Affiliation:
JILA / University of Colorado, Boulder CO 80309-0440, USA
F. Hill
Affiliation:
National Solar Observatory, Tucson AZ 85726-6732, USA
H. M. Antia
Affiliation:
Tata Institute of Fundamental Research, Mumbai 400005, India

Abstract

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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.

Type
Session II: Convection Zone and Local Area Helioseismology
Information
Symposium - International Astronomical Union , Volume 203: Recent Insights into the Physics of the Sun and Heliosphere: Highlights from Soho and Other Space Missions , 2001 , pp. 183 - 185
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

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.Google Scholar
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.Google Scholar