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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 7.

Current sheet and reconnection outflows. Left: normal image (bright corresponds to high intensities, dark to low). We artificially lowered the solar disk intensity to make the current sheet more distinguishable. Right: negative image (dark corresponds to high intensities, bright to low). Image was taken on April 17 at 12:38 UT. The dashed lines designate the position of the artificial slit. Coordinates are measured in arcseconds.

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