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A Critical Assessment of Nonlinear Force-Free Field Modeling of the Solar Corona for Active Region 10953

  • Authors: Marc L. DeRosa, Carolus J. Schrijver, Graham Barnes, K. D. Leka, Bruce W. Lites, Markus J. Aschwanden, Tahar Amari, Aurélien Canou, James M. McTiernan, Stéphane Régnier, Julia K. Thalmann, Gherardo Valori, Michael S. Wheatland, Thomas Wiegelmann, Mark C. M. Cheung, Paul A. Conlon, Marcel Fuhrmann, Bernd Inhester, and Tilaye Tadesse

DEROSA et al. 2009 The Astrophysical Journal 696 1780.

  • Provider: AAS Journals

Caption: Figure 5.

( a) Scatter diagram illustrating the mismatch between the values of α implied by the preprocessed Hinode/SOT–SP boundary data for all points having B z >0, and the values of α for field lines in the Wh model intersecting these same points. For a consistent boundary condition where the α-correspondence relation is satisfied, the values of α on each field line in the Wh solution (which are taken from the negative-polarity end of the field line) would match the measured value of α found at the positive-polarity end. ( b) The differential change dΦ/ dα in net flux Φ integrated over all points having α values greater than the abscissa. The unpreprocessed (red) and preprocessed (black) boundary data for AR 10953 are both shown. Data for which the α-correspondence relation holds have dΦ/ dα = 0.

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