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Paper detail

CME Acceleration as a Probe of the Coronal Magnetic Field

By 2050, we expect that CME models will accurately describe, and ideally predict, observed solar eruptions and the propagation of the CMEs through the corona. We describe some of the present known unknowns in observations and models that would need to be addressed in order to reach this goal. We also describe how we might prepare for some of the unknown unknowns that will surely become challenges.

preprint2020arXivOpen access
James Paul MasonPhillip C. ChamberlinThomas N. WoodsAndrew JonesAstrid M. VeronigKarin DissauerMichael KirkSunCET Team
astro-ph.SR
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James Paul MasonPhillip C. ChamberlinThomas N. WoodsAndrew JonesAstrid M. VeronigKarin DissauerMichael KirkSunCET Team

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