Skip to main content Accessibility help
×
Hostname: page-component-5c6d5d7d68-qks25 Total loading time: 0 Render date: 2024-08-19T23:18:35.307Z Has data issue: false hasContentIssue false

Introduction

Published online by Cambridge University Press:  25 January 2010

M. R. E. Proctor
Affiliation:
University of Cambridge
A. D. Gilbert
Affiliation:
University of Exeter
Get access

Summary

Magnetic fields are observed to exist wherever there is matter in the visible universe; they exist on planetary, stellar and galactic length-scales, indeed wherever there is a sufficiently large mass of rotating conducting fluid. Dynamo theory is that branch of fluid mechanics that seeks to explain both the origin of these magnetic fields, and the manner of their variation in space and time. The subject has exerted a profound challenge, and great advances have been made over the last few decades. Nevertheless, acute problems remain in relation to both planetary and stellar magnetism. The NATO Advanced Study Institute on Stellar and Planetary Dynamos, and the six-month Dynamo Theory Programme of the Isaac Newton Institute of which it formed part, set out both to review the present state of knowledge in this broad field, and to define the critical problems that now demand attention.

The problem of the origin of the Earth's magnetic field has challenged the imagination of great scientists of past centuries. Edmund Halley showed extraordinary prescience three hundred years ago when, in considering the possible causes of the secular variation of the geomagnetic field, he wrote:

“ … the external parts of the globe may well be reckoned as the shell, and the internal as a nucleus or inner globe included within ours, with a fluid medium between … only this outer Sphere having its turbinating motion some small matter either swifter or slower than the inner Ball.”

This view of the inner structure of the Earth was not confirmed till Jeffreys' discovery in 1926 of the liquid outer core and Bullen's discovery in 1946 of the solid inner core.

Type
Chapter
Information
Publisher: Cambridge University Press
Print publication year: 1994

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

Save book to Kindle

To save this book to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

  • Introduction
  • Edited by M. R. E. Proctor, University of Cambridge, A. D. Gilbert, University of Exeter
  • Book: Lectures on Solar and Planetary Dynamos
  • Online publication: 25 January 2010
  • Chapter DOI: https://doi.org/10.1017/CBO9780511624025.002
Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

  • Introduction
  • Edited by M. R. E. Proctor, University of Cambridge, A. D. Gilbert, University of Exeter
  • Book: Lectures on Solar and Planetary Dynamos
  • Online publication: 25 January 2010
  • Chapter DOI: https://doi.org/10.1017/CBO9780511624025.002
Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

  • Introduction
  • Edited by M. R. E. Proctor, University of Cambridge, A. D. Gilbert, University of Exeter
  • Book: Lectures on Solar and Planetary Dynamos
  • Online publication: 25 January 2010
  • Chapter DOI: https://doi.org/10.1017/CBO9780511624025.002
Available formats
×