Fast Solar Wind Driven by Parametric Decay Instability and Alfvn Wave Turbulence
125,22 €
This book discusses key theoretical aspects concerning the formation of the solar wind: the most essential building block in the heliosphere, in which planets orbit. To understand the influence of solar activity on planetary magnetospheres and atmospheres, we need to first understand the origin of the solar wind, which is still under debate.
Jetzt bei Ebay:
