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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 3.

Transverse-displacement–time diagrams of the Ca ii intensity across the spicule at the higher section of spicule trace. The transverse-displacement profile at each height is plotted as a red line with a strand of red diamonds. Vertical bars are used to mark the σ width on two sides. The sine-fitting results are shown as blue dashed lines. The average position is marked with a black dotted line. The yellow arrows represent the propagation of the transverse-displacement oscillation, and the green arrows denote the motion of the jet head.

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