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Turbulent Heating and Anisotropy in the Solar Wind

A Numerical Study

Victor Montagud-Camps

978-3-030-30383-9

2019
Edition 1
- Nominated as an outstanding PhD thesis by the Physics Department of Paris-Sud University, Orsay, France
- Proves for the first time, using direct numerical simulations, that turbulent heating is one of the main contributors to solar wind heating between 0.3 and 1AU
- Demonstrates that the observed turbulent wave vector anisotropy at 1AU is linked to turbulent anisotropy near the Sun, and to the imbalance of Alfvén wave populations
- Provides results that allow us to hypothesize on the properties of solar wind turbulence near the Sun, at the end of the so-called acceleration region of the wind, and which could be verified by Parker Solar Probe and Solar Orbiter missions
€180

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