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Fig. 1.


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Convergence of the AMR-CESE-MHD model respect to the grid resolutions. The red, blue and light blue lines denote the pressure profiles (P th: thermal pressure, P d: dynamic pressure, P m: magnetic pressure, P tot: total pressure) of Case 1 along Sun-Earth line when the interest regions are refined with first-level, second-level and third-level grids, respectively.

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