Magnetic Flux Cancelation as the Buildup and Trigger Mechanism for CME-Producing Eruptions in two Small Active Regions
Alphonse C. Sterling, Ronald L. Moore, and Navdeep K. Panesar

TL;DR
This study investigates how magnetic flux cancelation in small active regions leads to the buildup and eruption of flux ropes, causing coronal mass ejections, and links these processes to similar mechanisms in solar jets.
Contribution
It demonstrates that flux cancelation is a key mechanism in small active regions for building eruptive flux ropes, extending understanding of eruption triggers across different solar phenomena.
Findings
30% and 50% flux cancelation before eruptions
Flux cancelation builds sheared core fields/flux ropes
Erupting filaments form at cancelation sites
Abstract
We follow two small, magnetically isolated CME-producing solar active regions (ARs) from the time of their emergence until several days later, when their core regions erupt to produce the CMEs. In both cases, magnetograms show: (a) following an initial period where the poles of the emerging regions separate from each other, the poles then reverse direction and start to retract inward; (b) during the retraction period, flux cancelation occurs along the main neutral line of the regions; (c) this cancelation builds the sheared core field/flux rope that eventually erupts to make the CME. In the two cases, respectively 30% and 50% of the maximum flux of the region cancels prior to the eruption. Recent studies indicate that solar coronal jets frequently result from small-scale filaments eruptions, with those "minifilament" eruptions also being built up and triggered by cancelation of magnetic…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Astro and Planetary Science
