A first step in reconstructing the solar corona self-consistently with a magnetohydrostatic model during solar activity minimumP. Ruan, T. Wiegelmann, B. Inhester, T. Neukirch, S. K. Solanki and L. FengA&A, 481 3 (2008) 827-834DOI: https://doi.org/10.1051/0004-6361:20078834
