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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. 4.

Estimated horizontal velocity vectors, ﹩\boldsymbol{v}_{\perp ,h}﹩ (white arrows) plotted over ANMHD’s horizontal velocity vectors at ﹩t=0﹩, ﹩\boldsymbol{V}_{\perp ,h}﹩ (aqua arrows) for LMSAL’s LCT, FLCT, and DAVE (top to bottom), for ﹩\Delta t=250﹩ s. Vectors are shown only for pixels in which ﹩\vert B_{z}\vert > 2.5\% ﹩ of ﹩\mathrm{max}\,( \vert B_{z}\vert ﹩), and for clarity, only every third vector was plotted. Gray scale shows ﹩B_{z}﹩. Blue (red) contours show smoothed upflows (downflows) corresponding to 0.12 and 0.04 km s−1 upward (downward). (The width of the smoothing window was 3 pixels.)

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