The magnetic structure of surges in small-scale emerging flux regions
David MacTaggart, Salvo Guglielmino, Andrew Haynes, Radostin Simitev, and Francesca Zuccarello

TL;DR
This study models small-scale flux emergence to understand how magnetic reconnection influences the formation and direction of surges, revealing the impact of magnetic topology and ambient field asymmetry.
Contribution
It introduces three flux emergence models that demonstrate how magnetic reconnection and field geometry guide surges in active regions.
Findings
Distinct reconnection phases determine surge paths.
Complex topology leads to additional eruptions.
Ambient field asymmetry influences surge direction.
Abstract
Aims: To investigate the relationship between surges and magnetic reconnection during the emergence of small-scale active regions. In particular, to examine how the large-scale geometry of the magnetic field, shaped by different phases of reconnection, guides the flowing of surges. Methods: We present three flux emergence models. The first model, and the simplest, consists of a region emerging into a horizontal ambient field that is initially parallel to the top of the emerging region. The second model is the same as the first but with an extra smaller emerging region which perturbs the main region. This is added to create a more complex magnetic topology and to test how this complicates the development of surges compared to the first model. The last model has a non-uniform ambient magnetic field to model the effects of emergence near a sunspot field and impose asymmetry on the system…
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