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- W1597478519 abstract "This chapter discusses the basic ideas of dynamo theory, as applied to the natural dynamos occurring in planets and stars. The level is appropriate for a graduate student with an undergraduate background in electromagnetic theory and fluid dynamics. It also discusses mean field dynamo theory. It is divided into two areas: (1) the underlying theory of mean field dynamo theory, or MFDT, the conditions for its validity, its relationship to turbulence theory and its extension to include nonlinear effects and (2) the solutions of MFDT equations and the new types of dynamos they create: dynamo waves, ω dynamos and α2 dynamos. The chapter also reviews dynamical regimes. Saturation is poorly understood, and is probably different in different dynamical regimes. It focuses on three problems: (1) dynamo saturation in moderately rotating systems, example the Sun. (2) dynamo saturation in rapidly rotating systems, dominated by Coriolis force, example the Earth's core, and (3) dynamo saturation in experiments. It also discusses numerical methods for dynamos. Cartesian geometry and spherical geometry are the most commonly used." @default.
- W1597478519 created "2016-06-24" @default.
- W1597478519 creator A5034627679 @default.
- W1597478519 date "2008-01-01" @default.
- W1597478519 modified "2023-10-18" @default.
- W1597478519 title "Course 2 Dynamo theory" @default.
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- W1597478519 doi "https://doi.org/10.1016/s0924-8099(08)80006-6" @default.
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