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4.2.3 Probe the structure in deep layers of the Sun.

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3.1 Probe the tachocline at the base of the convection zone, where the dynamo is surmised to be situated.

4.2.3.2 Studies of convective, rotational and meridional flows.

4.2.3.3 MDI-like medium-l program

4.2.3.4 Stereoscopic helioseismology