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Tests and Comparisons of Velocity‐Inversion Techniques

  • Authors: B. T. Welsch, W. P. Abbett, M. L. DeRosa, G. H. Fisher, M. K. Georgoulis, K. Kusano, D. W. Longcope, B. Ravindra, and P. W. Schuck

Welsch et al. 2007 The Astrophysical Journal 670 1434.

  • Provider: AAS Journals

Caption: Fig. 13.

Pixel‐by‐pixel scatter plots comparing several methods’ (LMSAL’s LCT, FLCT, and DAVE; top to bottom) estimated normal Poynting flux with ANMHD’s, for ﹩\Delta t=250﹩ s. For each method, linear and rank‐order correlation coefficients are shown, as is the ratio of the integrated estimated Poynting flux to the integrated actual Poynting flux.

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