Turbulent dynamics of the solar wind

Turbulent dynamics of the solar wind

Le but de cette thèse est l'étude du développement de la turbulence dans le vent solaire entre 0.2 et 1 unité astronomique (UA) du soleil (i.e. l'orbite terrestre). L'étude est faite en résolvant numériquement les équations de la MHD après soustraction de l'écoulement moyen radia...

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Bibliographic Details
Main Author:	Montagud Camps, Victor
Other Authors:	Université Paris-Saclay (ComUE)
Language:	en
Published:	2018
Subjects:	Turbulence Magnétohydrodynamique (MHD) Vent Solaire Magnetohydrodynamics (MHD) Solar Wind
Online Access:	http://www.theses.fr/2018SACLS373/document

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