Three-dimensional, magnetohydrodynamic simulation of the solar wind acceleration from the coronal base to 0.1 au


Munehito Shoda, The University of Tokyo, Department of Earth and Planetary Science, Bunkyo-ku, Japan, Takeru Ken Suzuki, University of Tokyo, Tokyo, Japan, Mahboubeh Asgari-Targhi, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States and Takaaki Yokoyama, University of Tokyo, Department of Earth and Planetary Science, Bunkyo-ku, Japan
Back to: Fundamental Physics of the Solar Corona and Inner Heliosphere II