Abstract
We present a three-dimensional reconstruction of an eruption that occurred on 2010 April 3 using observations from SWAP on board PROBA2 and SECCHI on board STEREO. The event unfolded in two parts: an initial flow of cooler material confined to a height 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. © 2011. The American Astronomical Society.
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Seaton, D. B., Mierla, M., Berghmans, D., Zhukov, A. N., & Dolla, L. (2011). SWAP-SECCHI observations of a mass-loading type solar eruption. Astrophysical Journal Letters, 727(1 PART II). https://doi.org/10.1088/2041-8205/727/1/L10
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