Abstract
Editorial: The Role of Turbulence in the Solar Wind, Magnetosphere, Ionosphere Dynamics
Highlights
This Research Topic is dedicated to one of the most intriguing and least understood phenomena of space plasma physics: nearly collisionless turbulence
Ness et al (1964) analyzed the magnetic field measurements made by the IMP 1 satellite and reported the existence of the region of turbulence between the magnetopause and the bow shock known as the magnetosheath
Klimchuk and Antiochos argue that in the closed corona of the Sun the ubiquitous current sheets arise from the quasi-static twisting of flux tubes rather than from the action of dynamic turbulence
Summary
The Role of Turbulence in the Solar Wind, Magnetosphere, Ionosphere Dynamics This Research Topic is dedicated to one of the most intriguing and least understood phenomena of space plasma physics: nearly collisionless turbulence. Our Research Topic includes a set of works dedicated to the study of different types of turbulence in the heliosphere.
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