DIRECT EVIDENCE FOR A FAST CORONAL MASS EJECTION DRIVEN BY THE PRIOR FORMATION AND SUBSEQUENT DESTABILIZATION OF A MAGNETIC FLUX ROPE

By S. Patsourakos, A. Vourlidas, Guillermo Stenborg. 2012

162 citations recorded by the source corpus.

Magnetic flux ropes play a central role in the physics of coronal mass ejections (CMEs). Although a flux-rope topology is inferred for the majority of coronagraphic observations of CMEs, a heated debate rages on whether the flux ropes pre-exist or whether they are formed on-the-fly during the eruption. Here, we present a detailed analysis of extreme-ultraviolet observations of the formation of a flux rope during a confined flare followed about 7 hr later by the ejection of the flux rope and an eruptive flare. The two flares occurred during 2012 July 18 and 19. The second event unleashed a fast (>1000 km s−1) CME. We present the first direct evidence of a fast CME driven by the prior formation and destabilization of a coronal magnetic flux rope formed during the confined flare on July 18.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/27fc14a256f0f9d78f2dcd20f7f2683670344851

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In Astronomy and Astrophysics

  1. G. Aulanier
  2. Etienne Pariat
  3. Brigitte Schmieder
  4. P. Démoulin
  5. M. Janvier
  6. V. Bommier
  7. Wei Liu
  8. V. Petrosian

In Molecular Biology

  1. Etienne Pariat
  2. P. Démoulin
  3. Brigitte Schmieder
  4. G. Aulanier
  5. M. Janvier
  6. V. Petrosian
  7. Wei Liu
  8. Qingrong Chen

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