Figure 1 from CURRENT SHEET STRUCTURES OBSERVED BY THE TESIS EUV TELESCOPE DURING A FLUX ROPE ERUPTION ON THE SUN

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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 1.

Standard CME model. Left: CME before reconnection; right: CME after reconnection. Green indicates the hot plasma in the current sheet and reconnection outflows.

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