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Flaring Loop Motion and a Unified Model for Solar Flares

  • Authors: P. F. Chen, C. Fang, M. D. Ding, and Y. H. Tang

Chen et al. 1999 The Astrophysical Journal 520 853.

  • Provider: AAS Journals

Caption: Fig. 3.

y‐plots of ﹩j_{z}﹩ (z‐component of the current density) and ﹩\left(< \boldsymbol{hspsp}="0.167">\boldsymbol{j}\boldsymbol{\times} \boldsymbol{B}\right)_{y}﹩ (the y‐component of the magnetic force) along the y‐axis (﹩x=0﹩) in model A1 at ﹩t=30\tau _{\mathrm{A}\,}﹩. The solid line corresponds to ﹩j_{z}﹩, and the dotted line to ﹩\left(< \boldsymbol{hspsp}="0.167">\boldsymbol{j}\boldsymbol{\times} \boldsymbol{B}\right)_{y}﹩.

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