Lectures on Solar and Planetary Dynamos ( Publications of the Newton Institute )

Publication series :Publications of the Newton Institute

Author: M. R. E. Proctor; A. D. Gilbert  

Publisher: Cambridge University Press‎

Publication year: 1994

E-ISBN: 9780511885310

P-ISBN(Paperback): 9780521461429

Subject: P142.7 cosmic electrodynamics

Keyword: 数学模拟、近似计算

Language: ENG

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Lectures on Solar and Planetary Dynamos

Description

Dynamo theory, the study of the generation and maintenance of magnetic fields by fluid motions, is important in many areas of physics, ranging from stellar and galactic dynamics, through solar physics and geomagnetism, to reactor physics. This volume contains the lectures given by leading specialists, for an intensive course held at the Newton Institute, as part of a NATO Advanced Study Institute. The course was intended for beginning graduate students, so starts with background material, before leading on to describe areas closer to current research. Topics covered include planetary and solar dynamos, fast dynamos and the use of symmetry principles to derive evolution equations. Detailed bibliographies are provided. As the only modern introduction to the subject, this will be welcome reading for students in planetary and solar physics, plasma physics and astrophysics.

Chapter

1.4 Working Dynamos

1.5 Mean Field Electrodynamics

Solar and Stellar Dynamos

2.1 Introduction

2.2 Stellar Magnetic Activity

2.3 Solar Activity

2.4 The Origin of the Solar Cycle

2.5 Where is the Solar Dynamo?

2.6 Self-Consistent Nonlinear Dynamo Models

2.7 Mean Field Dynamos

2.8 Illustrative Models

2.9 Stellar Dynamos

Convection and Magnetoconvection in a Rapidly Rotating Sphere

3.1 Introduction

3.2 Scaling, Geometry and Governing Equations

3.3 Non-magnetic Convection

3.4 Effects of a Weak Imposed Magnetic Field

3.5 Instability of Toroidal Fields in the Magnetostrophic Limit

3.6 Resistive and Diffusionless Instabilities

3.7 Instabilities of the Magnetic Field

3.8 Conclusions

Solar Dynamos: Computational Background

4.1 Introduction

4.2 Small-scale and Large-scale Magnetic Fields

4.3 Convective versus Mean-Field Dynamos

4.4 Numerical Methods

4.5 Direct Simulation of a Dynamo

4.6 Turbulent Transport Coefficients

4.7 Mean-field Dynamos

4.8 The Solar Dynamo and Differential Rotation

4.9 Future Simulations

Energy Sources for Planetary Dynamos

5.1 Introduction

5.2 Tidal and Precessional Resonant Bifurcations

5.3 Application to the Planets

5.4 Convective Energy Sources for Planetary Dynamos

5.5 In Temporary Conclusion

Fast Dynamos

6.1 Introduction

6.2 The Cauchy Solution and Reference Fields

6.3 Linear Flows

6.4 Slow Dynamos

6.5 Rope Dynamos

6.6 Spatially Periodic Dynamos

Nonlinear Planetary Dynamos

7.1 Introduction

7.2 Taylor's Constraint and its Variations

7.3 Equilibration through the Geostrophic Flow

7.4 Hydrodynamic Dynamos

The Chaotic Solar Cycle

8.1 Preface

8.2 The Solar Tachocline

8.3 The Solar Oscillator

8.4 On/Off Intermittency

8.5 Solar Activity Waves

8.6 Final Remarks

The Nonlinear Dynamo and Model-Z

9.1 Introduction

9.2 Nonlinear Axisymmetric Geodynamo Models

9.3 Model-Z Geodynamo

9.4 Conclusion

Maps and Dynamos

10.1 Brief Review of Dynamo Problems

10.2 Map-dynamo Models

10.3 Pulsed Beltrami Wave Dynamos

10.4 Essentially One-dimensional Map Dynamos

10.5 Analysis of Finn-Ott and SFS Models

10.6 Summary

Bifurcations in Rotating Systems

11.1 Introduction

11.2 Origin of Precession

11.3 Mode Interactions in Rotating Systems

11.4 Discussion

Index

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