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Preface

Published online by Cambridge University Press:  05 March 2016

Madhulika Guhathakurta
Affiliation:
NASA/LWS program scientist, Heliophysics Division, Science Mission Directorate
Carolus J. Schrijver
Affiliation:
Lockheed Martin Solar and Astrophysics Laboratory
Frances Bagenal
Affiliation:
University of Colorado Boulder
Jan J. Sojka
Affiliation:
Utah State University
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Summary

Anyone who has ever seen a picture of Earth taken from deep space can be forgiven for thinking of these two words: “splendid isolation.” Surrounded by millions of miles of uninterrupted black, the fragile blue globe seems profoundly alone, disconnected from anything else.

Nothing could be further from the truth: Earth is profoundly connected to our star.

The bright blue disk is just the most obvious evidence. A non-stop flood of sunlight warms the planet, simultaneously allowing us to live and to see. Invisible connections are equally profound. Solar radiation puffs up our atmosphere, altering its structure and chemistry. Solar winds buffet our magnetosphere, lighting up polar skies with curtains of light, and driving currents of electricity through the soil below. Solar magnetism deflects cosmic rays, moderating the effect of the Galaxy on our tiny home in space.

Years ago, the study of the Sun–Earth connection was edgy stuff. Big Thinkers held the planet and the star to be a system. From this synthesis emerged many new ideas and a new discipline called “heliophysics.”

Now we know that they weren't thinking big enough. Like Earth, every world in the solar system is connected to its star. From the surface chemistry of Mercury, to the tattered atmosphere of Mars, to the flowing ices of Pluto, the fingerprints of solar activity may be found in all corners of the heliosphere.

In pop culture, people trace the “seven degrees of separation” between themselves and actor Kevin Bacon. Earth is connected much more closely to alien worlds. The central role of the Sun puts us just one degree of separation away from scores of planets, dwarf planets, moons, asteroids, and comets throughout the solar system. This proximity tells us something important: what we learn about those strange places, we also learn about ourselves.

The connectedness of things is the subject of this book: Active Stars, their Astropheres, and Impacts on Planetary Environments. In 13 graduate-level chapters, experts lay out new ideas about how stars carve out a place in the galaxy to shape their own solar systems. The chapters touch on subjects ranging from magnetic reconnection and magnetohydrodynamics to climate and aeronomy. It may be one of the most interdisciplinary textbooks ever written – at least in the physical sciences.

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  • Preface
  • Edited by Carolus J. Schrijver, Frances Bagenal, University of Colorado Boulder, Jan J. Sojka, Utah State University
  • Book: Heliophysics: Active Stars, their Astrospheres, and Impacts on Planetary Environments
  • Online publication: 05 March 2016
  • Chapter DOI: https://doi.org/10.1017/CBO9781316106778.001
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  • Preface
  • Edited by Carolus J. Schrijver, Frances Bagenal, University of Colorado Boulder, Jan J. Sojka, Utah State University
  • Book: Heliophysics: Active Stars, their Astrospheres, and Impacts on Planetary Environments
  • Online publication: 05 March 2016
  • Chapter DOI: https://doi.org/10.1017/CBO9781316106778.001
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.

  • Preface
  • Edited by Carolus J. Schrijver, Frances Bagenal, University of Colorado Boulder, Jan J. Sojka, Utah State University
  • Book: Heliophysics: Active Stars, their Astrospheres, and Impacts on Planetary Environments
  • Online publication: 05 March 2016
  • Chapter DOI: https://doi.org/10.1017/CBO9781316106778.001
Available formats
×