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Table A.2

Scattering matrix parameters for lunar analog, Martian analog, and water ice particles.

Par. JSC-1A MMS-2L Ice
488 nm 520 nm 647 nm 488 nm 640 nm -
D1 50(11) 42.7 (8.6) 28.9 (4.7) 100 (18) 181 (40) 117 (20)
d1 209 (36) 165 (31) 121 (16) 557 (83) 769 (140) 1692 (270)
δ1 1.706 (68) 1.694 (48) 1.78 (7) 1.749 (52) 1.396 (43) 2.469 (71)
R1 0.124 (34) 0.080 (13) 0.090 (36) 0.312 (59) 0.43 (5) 0.05 (1)
r1 8.0 (5.8) 308 (160) 20 (13) 3.1 (1.3) 1.23 (34) 88 (72)
ρ1 3.0 (1.2) 7.7 (1.3) 6.3 (2.5) 3.1 (1.1) 2.15 (77) 7.6 (1.6)
S1 0.092 (33) 0.111 (58) 0.089 (31) 0.138 (53) 0.109 (43) 0.089 (37)
s1 202 (110) 158 (56) 17 (11) 43 (24) 103 (69) 358 (160)
RMS 0.011 0.0091 0.0074 0.0053 0.0040 0.049

A1 −0.389 (81) 0.57 (14) 1.84 (17) 0.92 (21) 0.44 (21) −2.33 (22)
β1 1.51 (16) 1.15 (11) 1.78 (27) 1.15 (14) 1.71 (15) 1.126 (77)
γ1 2.17 (26) 8.53 (44) 6.59 (34) 6.68 (24) 7.91 (44) 2.52 (25)
H1 −0.07 (3) −0.215 (18) −1.00 (24) −1.22 (29) −0.55 (16) 1.42 (23)
h1 22.92 (51) 9.18 (24) 1.37 (25) 0.87 (25) 0.97 (32) 1.99 (24)
η1 4.58 (34) 4.05 (23) 3.1 (2) 1.98 (15) 1.87 (22) 2.309 (97)
K1 0.059 (18) −0.168 (53) −0.507 (98) −0.103 (58) −0.089 (73) 0.13 (2)
k1 8.17 (22) 26.53 (21) 6.98 (42) 79.70 (21) 20.33 (15) 602.72 (31)
K1 1.123 (93) 2.87 (17) 2.46 (24) 3.39 (28) 3.00 (43) 1.90 (12)
RMS 0.0041 0.0049 0.0046 0.0054 0.0043 0.011

D2 0.954 (13) 0.9802 (86) 0.9661 (74) 0.888 (17) 0.761 (35) 0.9948 (29)
δ2 2.79 (19) 2.58 (16) 2.68 (13) 2.84 (24) 5.65 (69) 1.024 (19)
R2 0.450 (17) 0.421 (22) 0.396 (19) 0.527 (25) 0.075 (61) −0.116 (53)
ρ2 4.7 (5) 5.34 (85) 4.04 (53) 3.56 (38) 6.68 (74) 1997.80 (77)
S2 0.03 (2) 0.036 (24) 0.045 (23) 0.034 (26) 0.24 (6) 0.470 (46)
S2 422.21 (69) 20.14 (68) 13.41 (71) 176.09 (93) 1.5 (5) 31.76 (57)
RMS 0.018 0.011 0.0063 0.018 0.019 0.076

D3 0.954 (13) 0.94 (2) 0.9661 (74) 0.850 (29) 0.865 (42) 0.99996 (~0)
δ3 1.19 (13) 1.112 (79) 3.86 (17) 1.22 (15) 5.72 (84) 1.025 (19)
R3 −0.832 (69) −1.3(1) −0.411 (16) −1.31 (12) −0.188 (85) −0.84000 (~0)
ρ3 1.52 (15) 1.910 (97) 4.63 (49) 1.81 (12) 7.0 (5) 6.95 (38)
S3 0.352 (66) 0.8(1) −0.031 (19) 0.75 (12) −0.128 (82) 0.407 (41)
RMS 0.019 0.014 0.013 0.014 0.026 0.022

S3 7.44 (39) 3.16 (38) 795.80 (78) 3.10 (43) 2(1) 21.68 (57)
A2 0.8 (2) 2.05 (18) 0.80 (13) 0.272 (38) 0.318 (52) −1.77 (16)
β2 2.45 (44) 2.00 (14) 2.05 (33) 1.70 (24) 2.36 (22) 1.61 (16)
γ2 2.43 (51) 3.13 (21) 1.72 (36) 1.61 (24) 1.156 (78) 2.92 (21)
H2 −0.038 (22) −0.039 (11) −0.124 (48) −0.022 (24) −0.069 (26) 0.031 (15)
h2 25.53 (45) 24.34 (38) 8.4 (3) 14.76 (42) 28.55 (29) 70.50 (49)
η2 2.40 (23) 1.53 (36) 1.5 (2) 1.37 (34) 3.81 (31) 1.49 (27)
K2 −0.0392 (83) −0.552 (81) −0.019 (11) −0.014 (12) −0.0146 (66) 0.057 (26)
k2 240.18 (31) 5.86 (27) 23.79 (45) 22.36 (34) 14.23 (55) 4000.29 (26)
K2 1.27 (13) 2.80 (18) 1.22 (14) 1.36 (25) 1.077 (64) 1.98 (36)
RMS 0.0069 0.0053 0.0053 0.0045 0.0039 0.022

D4 0.944 (26) 0.980 (13) 0.952 (14) 0.867 (41) 0.784 (31) 0.9951 (34)
δ4 4.97 (47) 3.70 (26) 3.99 (13) 6.58 (37) 7.47 (42) 1.064 (46)
R4 −0.241 (46) −0.176 (33) −0.174 (18) −0.460 (55) −0.179 (29) 0.08959 (~0)
ρ4 9.60 (27) 7.18 (75) 9.20 (74) 7.05 (37) 9.11 (49) 1.36 (19)
S4 0.280 (57) 0.260 (41) 0.290 (26) 0.339 (77) 0.549 (44) 0.184 (36)
S4 741.4 (9) 493.0 (1.4) 701.0 (1.1) 570.78 (49) 1064.5 (1.1) 4699.76 (85)
RMS 0.046 0.027 0.014 0.034 0.021 0.022

Notes. As in Table A.1 for the JSC-1A lunar analog sample at the wavelengths of 488 nm, 520 nm, and 647 nm, the MMS-2L Martian analog sample at the wavelengths of 488 nm and 640 nm, and for the numerically simulated water ice particles.

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