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- W1640034735 abstract "We have been developing a self-consistent 2D MHD steady-state model of the solar corona and solar wind. This model is empirically constrained by 2D maps of the effective temperature, , and heat flux, , as originally derived by Sittler and Guhathakurta or SG model. The SG model has been applied to Mark II K-coronameter data, Skylab, Spartan and SOHO/LASCO white light coronagraph data, plus plasma and magnetic field Ulysses data. Our model uses the MHD conservation equations of mass, momentum and energy with a multipole expansion of the coronal magnetic field up to octupole term as the initial state for the MHD solutions. At present our MHD solutions are confined between the coronal base at 1.03 RS and 5 RS and will be expanded to larger heliocentric distances in the future. In order to make our MHD solutions more tractable, we have fit smooth analytical functions to and derived from the data-driven SG model. We will present solutions under these conditions, some of the difficulties we have had to deal with and show the future direction of our research. eff T eff q eff T eff q" @default.
- W1640034735 created "2016-06-24" @default.
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- W1640034735 date "2006-01-01" @default.
- W1640034735 modified "2023-09-27" @default.
- W1640034735 title "2D MHD model of the solar corona and solar wind: Recent results" @default.
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