Does the tachocline show solar cycle related changes?

Physics

Scientific paper

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Scientific paper

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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