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Space Physics pp 135-211 | Cite as

Sun and Solar Wind: Plasmas in the Heliosphere

  • May-Britt Kallenrode
Chapter
Part of the Advanced Texts in Physics book series (ADTP)

Abstract

Plasmas in interplanetary space originate from the Sun, as do most of the disturbances and waves embedded in them. The solar atmosphere, the corona, extends as solar wind far beyond the orbit of the outermost planet, Pluto, filling a cavity in the interstellar medium called the heliosphere. The solar magnetic field, frozen-in into the solar wind, is carried out and wound up to Archimedian spirals by the Sun’s rotation. Fluctuations and waves on different scales are superimposed, sometimes steepening to collisionless shock waves. The solar wind and the frozen-in magnetic field change during the solar cycle due to systematic changes in solar properties and transient disturbances related to solar activity. Detailed accounts on solar physics and the physics of the interplanetary medium are given in e.g. [113, 484, 572], and the solar corona and the physics of solar activity are described in e.g. [9,193, 244, 291, 410, 420, 424].

Keywords

Solar Wind Solar Cycle Coronal Mass Ejection Coronal Hole Magnetic Cloud 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2004

Authors and Affiliations

  • May-Britt Kallenrode
    • 1
  1. 1.Fachbereich PhysikUniversität OsnabrückOsnabrückGermany

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