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arXiv · 1011.1144

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

Daniel B. Seaton·Marilena Mierla·David Berghmans·Andrei N. Zhukov·Laurent Dolla
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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.

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Daniel B. Seaton, Marilena Mierla, David Berghmans, Andrei N. Zhukov, Laurent Dolla. 2010-11-04. SWAP-SECCHI Observations of a Mass-Loading Type Solar Eruption. https://doi.org/10.1088/2041-8205%2F727%2F1%2Fl10

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