Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aspc..444..143w&link_type=abstract
5th international conference of numerical modeling of space plasma flows (astronum 2010). Proceedings of a 5th international con
Astronomy and Astrophysics
Astronomy
Scientific paper
We present a solar wind model based on a three-dimensional (3D) data-driven, time-dependent, magnetohydrodynamic (MHD) model. The inputs to the model are the measured line-of-sight (LOS) magnetic field of SOLIS and transverse velocity from the Global Oscillation Network Group (GONG) on the lower boundary without heating and momentum additions. The results show that both slow and fast components of the solar wind are produced without arbitrarily specifying additional heating and momentum due to the employment of multiple sets of observations. In addition, the global distribution of the coronal holes responsible for the formation of co-rotating interaction regions (CIRs) is also consistently presented.
Dryer Murray
Feng Xue-Shang
Hernandez Irene Gonzalez
Hill F. F.
Wang Ai-Hua
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