Space Weather

  • Oleg Novik
  • Feodor Smirnov
  • Maxim Volgin


In this chapter, we briefly describe the structure and dynamics of the plasma of the solar wind, which supplies solar energy to the plasmas of the earth’s geospheres, namely the magnetosphere and ionosphere. Then, geomagnetic storms, which develop there and disturb the physical fields of the underlying earth atmosphere, are discussed. We use the qualitative approach of the US Space Weather Prediction Center (SWPC), the National Oceanic and Atmospheric Administration (NOAA), Spacepedia, Wikipedia, and the National Aeronautic and Space Administration (NASA) to discuss these subjects, i.e., systems of partial differential equations (PDEs; e.g., ones describing magneto-hydrodynamics) are not applied in this chapter, though the processes described by them include most of the related physics. (We note that systems of PDEs are applied and/or investigated by us numerically and mathematically in Chaps.  1,  2,  3,  9,  10, and  11 of this book.)

The influences of geomagnetic storms (estimated by the planetary geomagnetic index Kp, which is described in this chapter) on the human brain and heart are considered in Chaps.  5,  6,  7, and  8 of this book.


Plasma Solar wind Magnetosphere Ionosphere Geomagnetic storm 


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Copyright information

© Springer Nature Switzerland AG 2019

Authors and Affiliations

  • Oleg Novik
    • 1
  • Feodor Smirnov
    • 1
  • Maxim Volgin
    • 1
  1. 1.IZMIRAN of the Russian Academy of SciencesMoscowRussia

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