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CURRENT SHEET STRUCTURES OBSERVED BY THE TESIS EUV TELESCOPE DURING A FLUX ROPE ERUPTION ON THE SUN

  • Authors: A. A. Reva, A. S. Ulyanov, and S. V. Kuzin

2016 The Astrophysical Journal 832 16.

  • Provider: AAS Journals

Caption: Figure 10.

Left: scanning of the Y-structure intensity. Black line indicates the intensity across the slit, red dashed line indicates background fit. Right: determination of the Y-structure thickness. Black line: intensity scan after background subtraction; dotted blue line: “main” Gaussian profile; dotted red line: Y-structure Gaussian profile; blue line: intensity fit (difference between the “main” and the Y-structure Gaussian profiles).

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