Download Stretch, Twist, Fold: The Fast Dynamo (Lecture Notes in by Stephen Childress PDF

By Stephen Childress

The learn of planetary or sun magnetic fields explains traditional magnetism as a phenomenon of magnetohydrodynamics. The kinematic dynamo idea, in particular the quick dynamo handled during this quantity, is slightly easier yet nonetheless it provides ambitious analytical difficulties relating to chaotic dynamics, for instance. This striking booklet offers the prestige of the idea, together with ideas of numerical simulations and modelling, in addition to a precis of effects to this point. the 1st 3 chapters introduce the matter and current examples of quickly dynamo motion in flows and maps. the remainder 9 chapters take care of numerous analytical methods and version structures. The booklet addresses astronomers and geophysicists, researchers and scholars alike.

Show description

Read or Download Stretch, Twist, Fold: The Fast Dynamo (Lecture Notes in Physics Monographs) PDF

Best atomic & nuclear physics books

Stretch, Twist, Fold: The Fast Dynamo (Lecture Notes in Physics Monographs)

The learn of planetary or sunlight magnetic fields explains normal magnetism as a phenomenon of magnetohydrodynamics. The kinematic dynamo thought, in particular the quick dynamo taken care of during this quantity, is a little less complicated yet nonetheless it offers bold analytical difficulties with regards to chaotic dynamics, for instance.

Introduction to the Theory of Collisions of Electrons with Atoms and Molecules

An figuring out of the collisions among micro debris is of significant value for the variety of fields belonging to physics, chemistry, astrophysics, biophysics and so forth. the current booklet, a concept for electron-atom and molecule collisions is built utilizing non-relativistic quantum mechanics in a scientific and lucid demeanour.

Theoretical Atomic Physics

This proven textual content comprises a sophisticated presentation of quantum mechanics tailored to the necessities of recent atomic physics. The 3rd variation extends the winning moment variation with a close therapy of the wave movement of atoms, and it additionally includes an advent to a few features of atom optics that are suitable for present and destiny experiments concerning ultra-cold atoms.

The Nuclear Many-Body Problem

This long-standing introductory textual content completely describes nuclear many-body idea, with an emphasis on technique and the technical features of the theories which have been used to explain the nucleus. Now on hand in a cheaper softcover version, the unique contents of "The Nuclear Many-Body challenge” offered here's meant for college kids with uncomplicated wisdom of quantum mechanics and a few figuring out of nuclear phenomena.

Extra resources for Stretch, Twist, Fold: The Fast Dynamo (Lecture Notes in Physics Monographs)

Sample text

We stress at once that few of these questions have been answered satisfactorily, and then only for very restrictive models. advective time-scale. In the case of the induction equation the diffusion time is L 2 1'TJ' In the present problem such usage would imply that some dynamos defined here as 'slow' would qualify as 'fast'. In a practical sense the distinction between a fast dynamo and a slow dynamo with, say, , rv II log E, is not essential. But it is worth indicating the origins of fast dynamo action in stretching flows by adopting the strict time-scale of the fluid, namely L I U.

6 we look at examples of three-dimensional steady flows. 2 Numerical Evidence for a Fast Dynamo in Otani's MW + Flow 33 view of dynamos, or even as dynamical systems (but see Feingold, Kadanoff & Piro 1988). Other possibilities include the random two- or three-dimensional flows studied in Chap. 11. 1 3 We call this the MW+ flow for brevity, meaning 'modulated waves, positive parity'. 14 Otani's modulation is one of many that might be considered by assigning general amplitudes a(t) and (3(t) to the waves, and so parameterising an oriented closed curve in the (a, (3)-plane.

7) We run the code until the fastest growing magnetic field eigenmode emerges and the growth rate settles down to ,(E, k). The solid line in Fig. 4. 4. 8. 8 and in Fig. 2 plot ,(E, k) against logiO liE. 39. From the computational evidence, the dynamo appears to be fast (Otani 1988, 1993). 2) for ,(E), can only increase the growth rate. 8 in Fig. 2, the corresponding eigenfunctions become wild in this limit. Fig. 3 shows eigenfunctions for decreasing values of E. We plot Re bx (x, y) at time t == 401r on a color scale with yellow I red for 36 2.

Download PDF sample

Rated 5.00 of 5 – based on 14 votes