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Excitation of Kink Waves Due to Small-Scale Magnetic Reconnection in the Chromosphere?

  • Authors: Jiansen He, Eckart Marsch, Chuanyi Tu, and Hui Tian

HE et al. 2009 The Astrophysical Journal 705 L217.

  • Provider: AAS Journals

Caption: Figure 2.

Diagrams of the transverse displacement vs. time for the Ca ii intensity across the spicule at the lower section of spicule trace. The transverse displacement profile at each height is plotted as a red line with a strand of red diamonds. The half length of each vertical bar represents a σ width, which is defined in the text. The blue dashed line in each panel is the sine-fitting result for the transverse displacement profile. The black-dotted line is placed at the average position.

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