V. Taylor-couette-ow and .. , The angular velocity of the lids and the inner cylinder is ? i = 1; the outer cylinder is motionless. A radial jet ows inward at the equator. Represented are the poloidal ow (vectors and streamlines) ?0.2 ? V r ? 0.3, and ?0, and the toroidal (or azimuthal), p.202

F. Taylor-couette-ow, V. I. , ?. =. , and .. , R e = 120, and A = 2.5. The lids and the inner cylinder rotate with angular speed ? i = 0.55; the outer cylinder is motionless. A radial jet ows inwards at the equator. Represented are the poloidal ow (vectors and streamlines, ?0.7 ? V r ? 1.4, ?1.1 ? V z ? 1.1, and the toroidal, p.204

R. Kinematic-dynamo, =. , and .. , Growthrate of Fourier mode m = 1 for the modied Taylor- Couette ow, V ? , as a function of ? for R m = 100 and R m = 200, p.205

. Kinematic, Magnetic eigenvector for Fourier mode m = 1 Represented in (a) to (f) are the radial, azimuthal, and vertical components, normalized by the square root of the magnetic energy, in two complementary planes, with 0 ? r ? 2, ?1 ? z ? 1 (the z?axis is on the left): for ? = 0

V. Kinematic-dynamo-of-ow, Growthrate of the Fourier mode m = 1 as a function of R m, p.207

R. Kinematic-dynamo-with-v-i-ow, =. , and .. , Growthrate of the Fourier mode m = 1 as a function of R m . ROT: rotating inner core; NO-ROT: non-rotating inner core (but inner wall rotates), p.207

V. Kinematic-dynamo-with-ow, R. , and =. , Magnetic eigenvector for Fourier mode m = 1 Represented in (a) to (f) are the radial, azimuthal, and vertical components, normalized by the square root of the magnetic energy, in two complementary planes: for ? = 0, ?0.9 ? H r ? 0.2 (every 0.1), ?1.4 ? H ? ? 0.35 (every 0.25) and ?0.6 ? H z ? 0.6 (every 0.1); for ? = ?, p.208

K. For-dierent-reynolds-numbers, R. , and ?. , 223 G.5 (Color online) Time evolution of the asymmetry ratio r a for dierent Reynolds numbers R e ? [700 224 G.6 (Color online) Time evolution of the asymmetry ratio r a at R e = 750 and R e = 800 to show the short period of oscillations (Color online) Time evolution of the magnetic energy M in the conducting uid (a) in the linear regime from t = 192 at R e = 1200 and various R m as indicated (in lin-log scale) and (b) in the nonlinear regime from t = 192 to t = 287, p.226, 1200.

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