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Table 1.
Model inputs varied in the Monte Carlo ensembles, grouped by the physical role in the EFR framework.
| Group | Parameters varied | Notes / description |
|---|---|---|
| Geometry / spatial scales | h0, sf, ratio | Eruption onset height (h0), footpoint separation (sf), and aspect ratio (ratio) controlling flux-rope geometry and expansion scaling. |
| Poloidal-flux injection profile | τ1, τ2, t1, t2, t3, q1 | Rise/decay timescales (τ1, τ2), timing markers (t1, t2, t3), and injection amplitude (q1) defining the prescribed dΦp/dt driver. |
| Magnetic-field initialization | Bp, Bt | Initial poloidal and toroidal field strengths setting the starting magnetic content of the rope. |
| Plasma density / mass loading | ncavity0, δ | Initial cavity number density (ncavity, 0) and prominence fall-off / residual factor (δ) controlling internal mass loading and its evolution. |
| Solar-wind background and coupling | vsw0, nsw0, Cd | Upstream solar-wind speed and density, and the drag coefficient controlling momentum exchange during propagation. |
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