Fig. 5 from Flaring Loop Motion and a Unified Model for Solar Flares

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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. 5.

Time profiles of magnetic reconnection rate (R) in model A1 (solid line) and model B (dotted line). ﹩R=d\psi _{n}/ dt﹩, where ﹩\psi _{n}﹩ is dimensionless, and the unit of t is ﹩\tau _{\mathrm{A}\,}﹩.

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