Solar Wind Turbulence

  • Victor Montagud-CampsEmail author
Part of the Springer Theses book series (Springer Theses)


Thanks to the deployment of satellite probes in the heliosphere since the 90s (Ulysses, Helios, ACE, Wind...), solar wind is one of the few examples of astrophysical plasmas in which in-situ measurements can be made. Since the launch of these probes, it has been possible to recover data from solar wind plasma using several types of instruments. From these in-situ measurements, it has been possible to study several properties of solar wind turbulence, such as the energy spectrum of magnetic fluctuations, turbulent anisotropy or turbulent heating. We will describe all these properties in the present chapter.


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© Springer Nature Switzerland AG 2019

Authors and Affiliations

  1. 1.Department of Surface and Plasma ScienceCharles UniversityPragueCzech Republic

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