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Magnetic Energy Storage and Conversion in the Solar Atmosphere

  • Chapter
Physics of the Sun

Part of the book series: Geophysics and Astrophysics Monographs ((GAAM,volume 25))

Abstract

Until man broke gravity’s shackles, now more than 20 years ago, our knowledge of the multifaceted role played by magnetic fields on the Sun was meager. The past few decades of steadily improving X-ray and ultraviolet observations above the atmosphere have fostered a corresponding growth in our understanding of the importance of magnetic energy conversion and release and magnetohydrodynamic activity to virtually all components of solar variability which affect our environment here on Earth. Every experimental improvement has brought us a closer and better view of the dynamic, sometimes violent, MHD and plasma phenomena which are now generally agreed to control the solar transition region, corona, solar wind, flares, spots, bright points, and spicules.

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Author information

Authors and Affiliations

  1. E. O. Hulburt Center for Space Research and Laboratory for Computational Physics, Naval Research Laboratory, Washington, DC, 20375, USA

    D. S. Spicer, J. T. Mariska & J. P. Boris

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  1. D. S. Spicer
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  2. J. T. Mariska
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  3. J. P. Boris
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Editor information

Editors and Affiliations

  1. Center for Space Science and Astrophysics, Stanford University, Stanford, California, USA

    Peter A. Sturrock

  2. High Altitude Observatory, National Center for Atmospheric Research, Boulder, Colorado, USA

    Thomas E. Holzer  & Dimitri M. Mihalas  & 

  3. Astronomy Department, University of California, Los Angeles, California, USA

    Roger K. Ulrich

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© 1985 Springer Science+Business Media Dordrecht

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Spicer, D.S., Mariska, J.T., Boris, J.P. (1985). Magnetic Energy Storage and Conversion in the Solar Atmosphere. In: Sturrock, P.A., Holzer, T.E., Mihalas, D.M., Ulrich, R.K. (eds) Physics of the Sun. Geophysics and Astrophysics Monographs, vol 25. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-9636-2_5

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  • DOI: https://doi.org/10.1007/978-94-010-9636-2_5

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