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A first step in reconstructing the solar corona self-consistently with a magnetohydrostatic model during solar activity minimum - MaRDI portal

A first step in reconstructing the solar corona self-consistently with a magnetohydrostatic model during solar activity minimum (Q3502359)

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A first step in reconstructing the solar corona self-consistently with a magnetohydrostatic model during solar activity minimum
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    A first step in reconstructing the solar corona self-consistently with a magnetohydrostatic model during solar activity minimum (English)
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    23 May 2008
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    Sun: corona - Sun: magnetic fields - magnetohydrodynamics (MHD)
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