Table 3: Wavelengths (in nm) exhibiting strongest polarization in the solar-like model. The numbers in parenthesis give the degree of polarization (relative to the local continuum).

100 G	1000 G	5000 G
1159.34 (7.18%)	525.02 (35.38%)	448.97 (44.36%)
846.83 (6.56%)	423.27 (34.63%)	420.66 (44.13%)
1449.77 (6.27%)	425.83 (34.21%)	411.17 (43.63%)
525.02 (5.94%)	524.75 (33.64%)	431.28 (43.37%)
1564.84 (5.78%)	408.08 (33.62%)	400.16 (43.24%)
1386.41 (5.74%)	513.14 (33.36%)	417.49 (43.11%)
1168.98 (5.71%)	461.33 (33.33%)	408.29 (43.02%)
1142.22 (5.45%)	454.59 (31.96%)	412.12 (42.67%)
1456.57 (5.45%)	550.67 (31.95%)	429.14 (42.65%)
513.14 (5.38%)	522.55 (31.89%)	457.10 (42.55%)
524.75 (5.37%)	448.56 (31.66%)	437.44 (42.55%)
525.01 (5.26%)	429.14 (31.10%)	438.92 (42.53%)
1399.74 (5.25%)	465.44 (30.81%)	405.55 (42.43%)