Table A.2
Influence of the turbulence on the mean fidelity of B-field mapping from polarized dust emission at λ = 0.8 mm in protostellar envelopes at different scales.
| msink | B-field recovery rates and σ [%] | |||
|---|---|---|---|---|
| [M⊙] | All scales | 30 – 100 au | 100 – 500 au | 500 – 1500 au |
| R1 | 97.5 2.4 | 70.9 7.5 | 85.7 12.0 | 93.1 7.2 |
| R6 | 91.9 4.5 | 70.7 13.2 | 82.0 10.1 | 87.8 10.5 |
Notes. Mean recovery rates at different scales for an error bar of 15°. The values have been averaged for all the evolutionary stages and projections for simulations R1 (non-turbulent) and R6 (turbulent) given in Table A.1. The values given in a smaller font correspond to the standard deviation.
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