**Table 3:** Model results for a planet at opposition (phase angle $\alpha =0^\circ$ ) with a semi-infinite Rayleigh-scattering atmosphere. The columns give the single-scattering albedo $\omega$ , the geometric albedo $A_{\rm g}$ , the disk-integrated radial polarization $\langle Q_{\rm r}/I\rangle$ , the line-integrated radial polarization for a line through the disk center, and the maximum radial polarization $Q_{\rm r}(r)/I(r)\vert _{\rm max}$ .
$\omega$	$A_{\rm g}$	$\langle Q_{\rm r}/I\rangle$	$\langle Q_{\rm r}/I\rangle_{\rm line}$	$Q_{\rm r}/I\vert _{\rm max}$
		[%]	[%]	[%]
1.00	0.796	2.73	1.64	7.7
0.99	0.638	3.29	2.03	8.1
0.95	0.489	3.48	2.19	7.9
0.90	0.398	3.35	2.13	7.4
0.80	0.291	2.90	1.86	6.3
0.60	0.171	2.01	1.29	4.3
0.40	0.096	1.24	0.80	2.6
0.20	0.042	0.57	0.37	1.2

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