NASA NTRS · 20060039416
The Swelling and Destabilization of a Coronal Mass Ejection (abstract)
Abstract
We will present and discuss data for a bugle that was particularly well observed. Apparently the swelling of the bugle and its destabilization were caused by the newly emerging flux and its interaction with the pre-existing active regions and coronal structures.
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Martin, S. F., Feynman, J.. 1993-12-06. The Swelling and Destabilization of a Coronal Mass Ejection (abstract). https://ntrs.nasa.gov/citations/20060039416
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