Turbulent Heating and Anisotropy in the Solar Wind, 1st ed. 2019 A Numerical Study Springer Theses Series
Auteur : Montagud-Camps Victor
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
Date de parution : 10-2020
Ouvrage de 123 p.
15.5x23.5 cm
Date de parution : 10-2019
Ouvrage de 123 p.
15.5x23.5 cm
Disponible chez l'éditeur (délai d'approvisionnement : 15 jours).
Prix indicatif 105,49 €
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