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A Reexamination of the Evidence for Reconnection Inflow

  • Authors: P. F. Chen, K. Shibata, D. H. Brooks, and H. Isobe

Chen et al. 2004 The Astrophysical Journal Letters 602 L61.

  • Provider: AAS Journals

Caption: Fig. 1.

Top: Evolution of the Fe XII 195 Å emission in observations. Bottom: Evolution of the magnetic field (solid lines), velocity (arrows), and Fe XII 195 Å emission intensity (gray scale) in the simulation. Threadlike structures are indicated by white thick arrows in both cases.

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