Three-dimensional MHD modeling of the global corona throughout solar cycle 23

Details Three-dimensional MHD modeling of the global corona throughout solar cycle 23 Three-dimensional MHD modeling of the global corona throughout solar cycle 23

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jgra..11303106h&link_type=abstract

Journal of Geophysical Research, Volume 113, Issue A3, CiteID A03106

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Solar Physics, Astrophysics, And Astronomy: Corona, Solar Physics, Astrophysics, And Astronomy: Magnetic Fields, Interplanetary Physics: Solar Cycle Variations (7536), Computational Geophysics: Modeling (4255)

Scientific paper

Based on the space-time conservation element and solution element (CESE) method, we have recently developed a novel 3D magnetohydrodynamic (MHD) model for the solar corona and interplanetary study. Our aim here is to describe the application of this new MHD model to study the global coronal magnetic structures by using the observed line-of-sight photospheric magnetic field from the Wilcox Solar Observatory (WSO) as boundary conditions. With this model, the magnetic structures of the global corona are obtained for fifteen Carrington Rotations (CRs) spanning solar cycle 23. The results illustrate how the shape and location of the heliospheric current sheet (HCS) and the coronal magnetic field configuration evolve during the course of the solar cycle. Comparison between our numerical results for the coronal magnetic structures and those from the standard potential field source surface (PFSS) model, with, in addition, white-light observations further validates this new MHD model. The source surface neutral lines calculated from the MHD and PFSS models generally match each other closely; however, differences occur at different phases in the solar cycle. The location of the HCS shows good overall agreement with the bright structures in the observed white-light intensity pattern, especially around solar minimum or well after solar maximum, and this result confirms that the observed white-light streamer structures originate from a single, large-scale plasma sheet located near the HCS.

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