All Tables

• Table 1: Stellar parameters used when generating synthetic data. Inversions with other values of i are described in Sect. 3.2.
• Table 2: Spectral lines that display similar behaviour to Fe I 6141.7 Å and Si I 6155.1 Å in the temperature range from 3750 K to 5250 K and that have previously been used for Doppler imaging.