Table 1.
Run parameters and simulations outcome at quasi-steady state.
| Run | βm, i | Accretion |  |
 |
 |
 |
 |
|---|---|---|---|---|---|---|---|
| A (Gagnier & Pejcha 2023) | ∞ | Yes | 0.016 | 0.034 | … | ... | … |
| A’ (Gagnier & Pejcha 2023) | ∞ | No | −0.026 | −0.042 | … | ... | … |
| B (This work) | 103 | Yes | 0.034 | 0.043 | 0.371 | 939 | 0.643 |
| B’ (This work) | 103 | No | −0.007 | −0.020 | 0.060 | 899 | 1.071 |
Notes. 
is computed using a lengthscale L corresponding to the typical scale of magnetic energy amplification (see Sect. 3.2.3), and V is taken as the averaged Alfvén speed in the region where 90% of magnetic energy amplification by line stretching occurs, averaged between t = 100Porb and t = 160Porb. Runs B and B’ in this study differ from the ones in Gagnier & Pejcha (2023).
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