WD 1703-267: Section of a diagram showing wavelengths magnetically split line components as a function of magnetic field strength B around 8.5 MG, with 2019-09-30 I (black) and V (red) spectra of WD 1703–267 superposed. Matching stellar spectra to split line components shows that field producing this spectrum has typical strength of ⟨|B|⟩ ≈8.5 MG. We note that wavelengths of blue σ components vary more rapidly with B than red components do.