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Solar Wind Sources and Their Variations over the Solar Cycle

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Solar Dynamics and Its Effects on the Heliosphere and Earth

Part of the book series: Space Sciences Series of ISSI ((SSSI,volume 22))

Abstract

In this paper I will briefly summarize the present status of our knowledge on the four different sorts of solar wind, their sources and their short- and long-term variations. First: the fast solar wind in high-speed streams that emerges from coronal hole regions. Second: the slow solar wind emerging from the non-active Sun near the global heliospheric current sheet above helmet streamers and underlying active regions. Third: the slow solar wind filling most of the heliosphere during high solar activity, emerging above active regions in a highly turbulent state, and fourth: the plasma expelled from the Sun during coronal mass ejections. The coronal sources of these different flows vary dramatically with the solar activity cycle.

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Authors and Affiliations

  1. Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Str. 2, 37191, Katlenburg-Lindau, Germany

    R. Schwenn

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  1. R. Schwenn
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Editors and Affiliations

  1. Laboratory for Atmospheric and Space Physics, Boulder, CO, USA

    D. N. Baker

  2. Max-Planck-Institute für extraterrestriche Physik, Garching, Germany

    B. Klecker

  3. Blackett Laboratory, Imperial College London, London, UK

    S. J. Schwartz

  4. Max-Planck Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany

    R. Schwenn

  5. International Space Science Institute (ISSI), Bern, Switzerland

    R. Von Steiger

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Schwenn, R. (2007). Solar Wind Sources and Their Variations over the Solar Cycle. In: Baker, D.N., Klecker, B., Schwartz, S.J., Schwenn, R., Von Steiger, R. (eds) Solar Dynamics and Its Effects on the Heliosphere and Earth. Space Sciences Series of ISSI, vol 22. Springer, New York, NY. https://doi.org/10.1007/978-0-387-69532-7_5

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