Physics
Scientific paper
Dec 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsh41a1617w&link_type=abstract
American Geophysical Union, Fall Meeting 2008, abstract #SH41A-1617
Physics
2101 Coronal Mass Ejections (7513), 2149 Mhd Waves And Turbulence (2752, 6050, 7836), 2752 Mhd Waves And Instabilities (2149, 6050, 7836)
Scientific paper
To understand how the particle (mass) flow transport across the magnetic boundary, a realistic example will be used to illustrate this process, which is to simulate the mass, magnetic flux, and energy transport from the sub-photosphere to the corona. The numerical simulation model that will be used in this paper is a newly developed data-driven three-dimensional global magnetohydrodynamic (MHD) model with the observed magnetic field and velocity field from GONG's data as the inputs at the photosphere. The difference between this new model and the model used in Wu, et al. 2005 is to include the effects of radiation and the transition region. Numerical simulation results to be presented are mass, total magnetic flux, and energy transport through photosphere to the corona, also the solar wind for the period of Halloween event.
Gonzáles-Hernández I.
Hill F. F.
Wang Anzhong
Wu Seongho
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