Astronomy and Astrophysics – Astronomy
Scientific paper
May 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.9106h&link_type=abstract
American Astronomical Society Meeting 210, #91.06; Bulletin of the American Astronomical Society, Vol. 39, p.205
Astronomy and Astrophysics
Astronomy
Scientific paper
The quasi-steady states of the three-dimensional global solar corona obtained with the time-dependent MHD simulation are presented. The synchronic frame format of solar magnetic field and the SOHO/EIT-based coronal temperature map are used as the boundary constraints, so that the pressure balance between the coronal plasma and magnetic field will be realistically simulated and thus the obtained three-dimensional simulation data will better represent the structures of the solar coronal at the time of interest. Our MHD code employs the concept of the projected normal characteristic method to include these measurement-based data as the sub-Alfvenic numerical boundary conditions without numerical instability.
Benevolenskaya Elena E.
Hayashi Keiji
Liu Ya-Ying
Zhao Xiaopeng
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