Table A.2
Degree of polarisation PE in our bandpasses corrected for lunar depolarisation.
ID | αMoon | ![]() |
![]() |
![]() |
![]() |
![]() |
|
---|---|---|---|---|---|---|---|
B.1 | 140.0 | 0.176(0.007) | 34.4(0.1)![]() |
22.7(0.1)![]() |
19.1(0.1)![]() |
16.8(0.4)![]() |
|
B.2 | 138.5 | 0.177(0.006) | 40.3(0.2)![]() |
26.3(0.1)![]() |
21.7(0.1)![]() |
16.9(0.3)![]() |
|
B.3 | 138.5 | 0.177(0.006) | 39.6(0.1)![]() |
26.7(0.1)![]() |
22.0(0.1)![]() |
17.8(0.4)![]() |
|
B.4 | 140.5 | 0.179(0.007) | 36.1(0.1)![]() |
24.8(0.1)![]() |
21.8(0.1)![]() |
19.7(0.5)![]() |
|
B.5 | 137.5 | 0.179(0.007) | 34.4(0.3)![]() |
24.2(0.1)![]() |
22.0(0.1)![]() |
20.4(0.8)![]() |
|
E.1 | 110.0 | 0.174(0.007) | 14.6(0.1)![]() |
9.7(0.0)![]() |
7.0(0.0)![]() |
4.8(0.1)![]() |
|
E.2 | 113.0 | 0.175(0.007) | 21.2(0.1)![]() |
13.7(0.1)![]() |
9.5(0.1)![]() |
6.0(0.1)![]() |
|
E.4 | 118.0 | 0.179(0.007) | 26.6(0.1)![]() |
17.5(0.1)![]() |
12.2(0.1)![]() |
7.4(0.2)![]() |
|
E.6 | 118.0 | 0.183(0.007) | 25.9(0.6)![]() |
17.3(0.1)![]() |
12.4(0.1)![]() |
7.9(0.2)![]() |
|
G.1 | 103.0 | 0.179(0.010) | 37.2(0.5)![]() |
30.0(0.5)![]() |
22.0(0.7)![]() |
18.6(0.7)![]() |
|
G.2 | 99.0 | 0.179(0.010) | 38.5(0.2)![]() |
29.5(0.2)![]() |
22.6(0.2)![]() |
19.8(0.3)![]() |
|
G.4 | 98.0 | 0.177(0.012) | 33.0(0.4)![]() |
24.5(0.2)![]() |
21.3(0.1)![]() |
18.6(0.3)![]() |
|
G.5 | 93.0 | 0.176(0.012) | 31.3(0.3)![]() |
23.9(0.3)![]() |
17.2(0.3)![]() |
14.3(0.7)![]() |
|
G.7 | 90.0 | 0.174(0.012) | 13.8(0.1)![]() |
11.2(0.1)![]() |
9.1(0.1)![]() |
10.2(0.2)![]() |
|
G.9 | 90.0 | 0.173(0.013) | 13.6(0.1)![]() |
11.2(0.1)![]() |
8.8(0.1)![]() |
8.0(0.6)![]() |
|
H.1 | 87.0 | 0.171(0.014) | 14.0(0.2)![]() |
12.8(0.1)![]() |
11.9(0.1)![]() |
10.5(0.1)![]() |
|
H.2 | 90.0 | 0.171(0.014) | 17.4(0.1)![]() |
11.7(0.1)![]() |
8.4(0.1)![]() |
5.7(0.2)![]() |
|
H.3 | 90.0 | 0.170(0.015) | 17.6(0.4)![]() |
12.7(0.1)![]() |
9.5(0.1)![]() |
7.1(0.2)![]() |
|
H.4 | 97.0 | 0.170(0.015) | 24.6(0.1)![]() |
17.4(0.1)![]() |
11.5(0.1)![]() |
7.0(0.2)![]() |
|
H.5 | 97.0 | 0.169(0.014) | 23.6(0.2)![]() |
17.2(0.2)![]() |
12.0(0.2)![]() |
7.5(0.3)![]() |
|
H.6 | 97.0 | 0.169(0.014) | 23.5(0.1)![]() |
16.3(0.1)![]() |
11.3(0.1)![]() |
6.9(0.2)![]() |
|
H.7 | 97.0 | 0.168(0.014) | 21.4(0.2)![]() |
14.3(0.1)![]() |
9.8(0.1)![]() |
6.0(0.2)![]() |
|
I.1 | 103.0 | 0.168(0.014) | 11.4(0.1)![]() |
9.5(0.0)![]() |
8.5(0.0)![]() |
7.5(0.2)![]() |
|
I.2 | 106.0 | 0.168(0.014) | 15.9(0.1)![]() |
10.5(0.0)![]() |
7.6(0.0)![]() |
5.1(0.1)![]() |
|
I.3 | 109.0 | 0.168(0.014) | 15.4(0.1)![]() |
10.4(0.0)![]() |
7.7(0.0)![]() |
5.3(0.1)![]() |
|
I.4 | 110.0 | 0.169(0.014) | 19.7(0.1)![]() |
12.8(0.0)![]() |
9.2(0.1)![]() |
5.9(0.1)![]() |
|
I.5 | 112.0 | 0.169(0.014) | 20.0(0.1)![]() |
13.2(0.1)![]() |
9.7(0.1)![]() |
6.5(0.1)![]() |
|
I.6 | 115.0 | 0.170(0.014) | 20.4(0.1)![]() |
13.7(0.1)![]() |
10.0(0.1)![]() |
6.7(0.2)![]() |
|
J.1 | 107.0 | 0.170(0.014) | 5.9(2.2)![]() |
8.5(0.7)![]() |
9.8(1.0)![]() |
10.3(1.4)![]() |
|
J.2 | 111.0 | 0.170(0.014) | 10.5(0.1)![]() |
7.8(0.0)![]() |
6.3(0.0)![]() |
5.3(0.1)![]() |
|
J.3 | 111.0 | 0.170(0.014) | 11.2(0.2)![]() |
7.9(0.1)![]() |
6.5(0.1)![]() |
5.2(0.2)![]() |
|
J.3-1 | 111.0 | 0.170(0.014) | 10.6(0.1)![]() |
8.0(0.2)![]() |
7.1(0.1)![]() |
6.7(0.1)![]() |
|
J.3-2 | 111.0 | 0.170(0.014) | 12.4(0.2)![]() |
9.8(0.1)![]() |
7.6(0.1)![]() |
6.6(0.1)![]() |
|
J.3-3 | 111.0 | 0.170(0.014) | 12.5(0.1)![]() |
9.9(0.1)![]() |
7.7(0.1)![]() |
6.8(0.1)![]() |
|
J.3-4 | 111.0 | 0.170(0.014) | 10.5(0.2)![]() |
7.9(0.1)![]() |
7.0(0.1)![]() |
6.7(0.1)![]() |
|
J.4 | 109.0 | 0.171(0.014) | 16.9(0.1)![]() |
11.3(0.1)![]() |
8.3(0.1)![]() |
5.5(0.2)![]() |
|
J.5 | 109.0 | 0.171(0.014) | 18.2(0.3)![]() |
12.1(0.2)![]() |
8.9(0.2)![]() |
5.9(0.2)![]() |
|
K.1 | 112.0 | 0.171(0.014) | 12.6(1.7)![]() |
11.3(0.5)![]() |
11.5(0.7)![]() |
9.9(2.6)![]() |
|
K.2 | 112.0 | 0.171(0.014) | 18.9(0.1)![]() |
13.5(0.1)![]() |
10.3(0.0)![]() |
7.6(0.1)![]() |
|
K.3 | 112.0 | 0.172(0.014) | 19.0(0.3)![]() |
13.5(0.2)![]() |
10.4(0.1)![]() |
7.7(0.2)![]() |
Notes. The determination of rotation angle αMoon of the moon with respect to the acquisition images and mean albedo for each observed region are explained in the text. Statistical errors of PE
(in brackets) are calculated from the null-profiles. Systematic errors of
PE are derived from the systematic errors to determine the lunar albedo
.
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