Abstract
It has been conjectured that the eruption of a solar prominence can be inhibited if a much larger scale, arched magnetic field straddles the prominence and effectively straps it down. We have demonstrated this effect in a laboratory experiment where a vacuum strapping field acts on a scaled simulation of a solar prominence. The required magnitude of the strapping field is in good agreement with a theoretical model that takes into account the full three-dimensional magnetic topology.
Cite
CITATION STYLE
Hansen, J. F., & Bellan, P. M. (2001). Experimental Demonstration of How Strapping Fields Can Inhibit Solar Prominence Eruptions. The Astrophysical Journal, 563(2), L183–L186. https://doi.org/10.1086/338736
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