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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. 9.

Pixel‐by‐pixel scatter plots of several methods’ (LMSAL’s LCT, FLCT, and DAVE; top to bottom) estimates of ﹩[ {\boldsymbol{\nabla}} \boldsymbol{\times} ( \boldsymbol{v}_{\perp }\boldsymbol{\times} \boldsymbol{B}) ] {\boldsymbol{\cdot}} \hat{\boldsymbol{z}}﹩ for ﹩\Delta t=250﹩ s, which should match ﹩\Delta B_{z}/ \Delta t﹩ assuming ideal MHD.

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