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SWAP-SECCHI Observations of a Mass-Loading Type Solar Eruption

Solar and Stellar Astrophysics 2015-05-20 v1 Space Physics

Abstract

We present a three-dimensional reconstruction of an eruption that occurred on 3 April 2010 using observations from SWAP onboard PROBA2 and SECCHI onboard STEREO. The event unfolded in two parts: an initial flow of cooler material confined to low in the corona, followed by a flux rope eruption higher in the corona. We conclude that mass off-loading from the first part triggered a rise, and, subsequently, catastrophic loss of equilibrium of the flux rope.

Keywords

Cite

@article{arxiv.1011.1144,
  title  = {SWAP-SECCHI Observations of a Mass-Loading Type Solar Eruption},
  author = {Daniel B. Seaton and Marilena Mierla and David Berghmans and Andrei N. Zhukov and Laurent Dolla},
  journal= {arXiv preprint arXiv:1011.1144},
  year   = {2015}
}

Comments

3 figures

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