Abstract
The tachocline at the base of the convection zone is generally believed to be the seat of the solar dynamo. Here we investigate whether the tachocline shows any detectable change using several 72 day time-series of the Michelson Doppler Imager (MDI) Medium-l data. We do not find any clear evidence of change with time.
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Antia, H. M., Basu, S., and Chitre, S. M.: 1998, Monthly Notices Royal Astron. Soc. 298, 543.
Basu, S.: 1997, Monthly Notices Royal Astron. Soc. 288, 572.
Basu, S. and Antia, H. M.: 1998, in Korzennik, S. and Wilson, A. (eds.) Proc. SOHO 6/GONG 98 Workshop, Structure and Dynamics of the Sun and Sun-like Stars, ESA SP-418, Noordwijk, p. 711.
Charbonneau, P., Christensen-Dalsgaard, J., Henning, R., Schou, J., Thompson, M. J., and Tomczyk, S.: 1997, in Provost, J. and Schmieder, F.-X. (eds.), IAU Symp. 181, Sounding Solar and Stellar Interiors, Posters Volume, p. 161.
Gilman, P. A. and Fox, P. A.: 1997, Astrophys. J. 484, 439.
Kosovichev, A. G.: 1996, Astrophys. J. 469, L61.
Schou, J.: 1999, Astrophys. J. 523, L181.
Schou, J., Antia, H. M., Basu, S. et al.: 1998, Astrophys. J. 505, 390.
Weiss, N. O.: 1994, in Proctor, M. R. E, and Gilbert, A. D. (eds.), Lectures on Solar and Planetary Dynamo, Cambridge University. Press, Cambridge, p. 59.
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Basu, S., Schou, J. Does the tachocline show solar cycle related changes?. Solar Physics 192, 481–486 (2000). https://doi.org/10.1023/A:1005231509224
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DOI: https://doi.org/10.1023/A:1005231509224