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

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.

preprint2010arXivOpen access
Daniel B. SeatonMarilena MierlaDavid BerghmansAndrei N. ZhukovLaurent Dolla
physics.space-phastro-ph.SR
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Daniel B. SeatonMarilena MierlaDavid BerghmansAndrei N. ZhukovLaurent Dolla

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