In this work the authors draw upon their expertise in geophysical
and astrophysical MHD to explore the motion of electrically
conducting fluids, the so-called dynamo effect, and describe the
similarities and differences between different magnetized objects.
They also explain why magnetic fields are crucial to the formation
of the stars, and discuss promising experiments currently being
designed to investigate some of the relevant physics in the
laboratory. This interdisciplinary approach will appeal to a wide
audience in physics, astrophysics and geophysics.
This second edition covers such additional topics as small-scale
dynamos, while also presenting the latest results and
experiments.
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