UID:
almafu_9959327278302883
Format:
1 online resource (x, 346 pages) :
,
illustrations (some color)
ISBN:
9783527648924
,
3527648925
,
9783527648955
,
352764895X
,
9783527648948
,
3527648941
,
3527410341
,
9783527410347
,
9781299804197
,
1299804195
Content:
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.
Note:
Differential rotation of stars -- Radiation zones : magnetic stability and rotation -- Quasi-linear theory of driven turbulence -- The galactic dynamo -- The magnetorotational instability (MRI) -- The Taylor instability (TI) -- Magentic spherical Couette flow.
Additional Edition:
Print version: ISBN 9783527410347
Language:
English
Keywords:
Electronic books.
;
Electronic books.
;
Electronic books.
URL:
https://onlinelibrary.wiley.com/doi/book/10.1002/9783527648924
URL:
https://onlinelibrary.wiley.com/doi/book/10.1002/9783527648924
URL:
https://onlinelibrary.wiley.com/doi/book/10.1002/9783527648924
