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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. 2.

Pixel‐by‐pixel scatter plots of several methods’ (LMSAL’s LCT, FLCT, and DAVE; top to bottom) estimates of the flux transport rate, ﹩\boldsymbol{u}B_{z}﹩, defined in eq. (3), with ANMHD’s flux transport rate, ﹩\boldsymbol{U}B_{z}﹩, over the shortest time interval between data dumps, ﹩\Delta t=250﹩ s. Blue and red are used to distinguish x‐ and y‐components, respectively. For each method, nonparametric Spearman rank‐order correlation coefficients and linear (Pearson) correlation coefficients are shown for both components of the flux transport velocity.

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