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3 - The heliosphere

Published online by Cambridge University Press:  05 June 2012

Mark Moldwin
Affiliation:
University of Michigan, Ann Arbor
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Summary

The heliosphere is defined as the region of interplanetary space where the solar wind is flowing supersonically.

Dessler, A.J. Reviews of Geophysics, 5, 33, 1967. The first use of the term heliosphere in the scientific literature.

Key concepts

  • plasma

  • solar wind

  • heliosphere

  • interplanetary magnetic field

  • coronal mass ejection

  • cosmic rays

Introduction

Sunlight, which bathes Earth with heat and light, is only part of the energy that flows constantly from the Sun. Ionized gas (plasma) and magnetic field are continuously expelled as solar wind, as well. Solar wind was discovered in the 1950s when it was noticed that the plasma tail of a comet always points away from the Sun, even when the comet is moving back towards deep space. Figure 3.1 shows a schematic of a typical comet and its tail at different points in its orbit around the Sun. A comet tail is made up of cometary material that has been heated by sunlight as it gets close to the Sun and has escaped from the nucleus. The glowing cloud of neutral and ionized gas and dust around the nucleus is called the coma. The material in the coma is then “blown” back away from the Sun. Creation of a comet tail requires not only sunlight, but also the energy and momentum of a gas flowing supersonically away from the Sun, the solar wind.

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Publisher: Cambridge University Press
Print publication year: 2008

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  • The heliosphere
  • Mark Moldwin, University of Michigan, Ann Arbor
  • Book: An Introduction to Space Weather
  • Online publication: 05 June 2012
  • Chapter DOI: https://doi.org/10.1017/CBO9780511801365.004
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  • The heliosphere
  • Mark Moldwin, University of Michigan, Ann Arbor
  • Book: An Introduction to Space Weather
  • Online publication: 05 June 2012
  • Chapter DOI: https://doi.org/10.1017/CBO9780511801365.004
Available formats
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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.

  • The heliosphere
  • Mark Moldwin, University of Michigan, Ann Arbor
  • Book: An Introduction to Space Weather
  • Online publication: 05 June 2012
  • Chapter DOI: https://doi.org/10.1017/CBO9780511801365.004
Available formats
×