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Observations of Reconnection Flows in a Flare on the Solar Disk

  • Authors: Juntao Wang, P. J. A. Simões, N. L. S. Jeffrey, L. Fletcher, P. J. Wright, and I. G. Hannah

2017 The Astrophysical Journal Letters 847 L1.

  • Provider: AAS Journals

Caption: Figure 5.

Model field at 00:04 UT just before the arcade eruption and the flare, derived from the PFSS package of Solarsoft, whose perspective has been rotated to 04:50 UT in order to compare with the extended blueshift region observed by EIS in Figure 3(d). It shows a narrow open-field corridor between two closed-field domains. The open-field corridor extends northward to a coronal hole. The blue dashed box shows the same region as the bottom left corner enclosed by the dashed line in Figure 3.

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