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1 - Introduction

Published online by Cambridge University Press:  06 July 2010

T. J. M. Boyd
Affiliation:
University of Essex
J. J. Sanderson
Affiliation:
University of St Andrews, Scotland
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Summary

Introduction

The plasma state is often referred to as the fourth state of matter, an identification that resonates with the element of fire, which along with earth, water and air made up the elements of Greek cosmology according to Empedocles.† Fire may indeed result in a transition from the gaseous to the plasma state, in which a gas may be fully or, more likely, partially ionized. For the present we identify as plasma any state of matter that contains enough free charged particles for its dynamics to be dominated by electromagnetic forces. In practice quite modest degrees of ionization are sufficient for a gas to exhibit electromagnetic properties. Even at 0.1 per cent ionization a gas already has an electrical conductivity almost half the maximum possible, which is reached at about 1 per cent ionization.

The outer layers of the Sun and stars in general are made up of matter in an ionized state and from these regions winds blow through interstellar space contributing, along with stellar radiation, to the ionized state of the interstellar gas. Thus, much of the matter in the Universe exists in the plasma state. The Earth and its lower atmosphere is an exception, forming a plasma-free oasis in a plasma universe. The upper atmosphere on the other hand, stretching into the ionosphere and beyond to the magnetosphere, is rich in plasma effects.

Solar physics and in a wider sense cosmic electrodynamics make up one of the roots from which the physics of plasmas has grown; in particular, that part of the subject known as magnetohydrodynamics – MHD for short - was established largely through the work of Alfvén.

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Publisher: Cambridge University Press
Print publication year: 2003

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  • Introduction
  • T. J. M. Boyd, University of Essex, J. J. Sanderson, University of St Andrews, Scotland
  • Book: The Physics of Plasmas
  • Online publication: 06 July 2010
  • Chapter DOI: https://doi.org/10.1017/CBO9780511755750.002
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  • Introduction
  • T. J. M. Boyd, University of Essex, J. J. Sanderson, University of St Andrews, Scotland
  • Book: The Physics of Plasmas
  • Online publication: 06 July 2010
  • Chapter DOI: https://doi.org/10.1017/CBO9780511755750.002
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
  • T. J. M. Boyd, University of Essex, J. J. Sanderson, University of St Andrews, Scotland
  • Book: The Physics of Plasmas
  • Online publication: 06 July 2010
  • Chapter DOI: https://doi.org/10.1017/CBO9780511755750.002
Available formats
×