Abstract: Three-dimensional MHD simulation of solar wind using a new boundary treatment: Comparison with in-situ data at Earth (AGU Fall Meeting 2018)

Three-dimensional MHD simulation of solar wind using a new boundary treatment: Comparison with in-situ data at Earth

Fang Shen¹, Zicai Yang², Jie Zhang³, Wenwen Wei² and Xueshang Feng², (1)National Space Science Center, CAS, Beijing, China, (2)National Space Science Center, Beijing, China, (3)George Mason University, Department of Physics and Astronomy, Fairfax, United States

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