| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 94.84 | 618.89 | 50.61 | 330.58 | 17.27 | 168.41 | 15.46 | 317.11 | 0.3741 | -389.2 | -258.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.36 | 0.00 | 1.29 | 11.11 | 176.77 | 23.82 | 292.65 | 0.4312 | -765.0 | -648.3 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 15.09 | 177.19 | 24.23 | 300.50 | 0.4619 | -779.0 | -593.1 | |
| 0.00 | 0.82 | 0.00 | 0.44 | 14.22 | 173.51 | 20.56 | 302.64 | 0.4060 | -755.0 | -583.4 | |
| 0.00 | 1.54 | 0.00 | 0.87 | 22.58 | 172.79 | 19.84 | 318.76 | 0.4772 | -700.0 | -521.1 | |
| 0.00 | 1.27 | 0.00 | 0.71 | 22.12 | 172.48 | 19.53 | 318.50 | 0.4692 | -768.0 | -604.1 | |
| 0.00 | 1.00 | 0.00 | 0.54 | 16.63 | 171.54 | 18.58 | 310.24 | 0.4017 | 777.0 | 648.5 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 15.56 | 171.40 | 18.44 | 308.26 | 0.3898 | -672.0 | -614.0 | |
| 0.00 | 1.36 | 0.00 | 0.75 | 20.07 | 171.10 | 18.15 | 317.19 | 0.4324 | -836.0 | -589.1 | |
| 0.00 | 1.72 | 0.00 | 0.91 | 13.47 | 170.13 | 17.18 | 305.48 | 0.3542 | -766.0 | -665.7 | |
| 0.00 | 2.18 | 0.00 | 1.15 | 12.67 | 169.72 | 16.76 | 304.15 | 0.3415 | -811.0 | -609.8 | |
| 77.14 | 486.82 | 41.40 | 261.27 | 17.27 | 169.66 | 16.71 | 314.43 | 0.3860 | -1573.8 | -449.9 | |
| 0.82 | -11.00 | 0.44 | -11.00 | 18.00 | 169.40 | 16.44 | 316.26 | 0.3910 | -1011.3 | 999999 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 12.90 | 168.53 | 15.57 | 306.64 | 0.3275 | -820.0 | -655.4 | |
| 0.00 | 1.00 | 0.00 | 0.54 | 18.39 | 168.73 | 15.78 | 318.11 | 0.3881 | -343.0 | -211.3 | |
| 0.00 | 2.09 | 0.00 | 1.09 | 14.66 | 166.50 | 13.55 | 314.72 | 0.3203 | -834.0 | -647.4 | |
| 0.00 | 3.27 | 0.00 | 1.74 | 18.34 | 166.57 | 13.62 | 322.06 | 0.3650 | 854.0 | 652.4 | |
| 0.00 | 2.09 | 0.00 | 1.10 | 17.11 | 166.41 | 13.45 | 320.09 | 0.3481 | 719.0 | 509.4 | |
| 0.00 | 2.09 | 0.00 | 1.09 | 14.47 | 166.20 | 13.24 | 314.92 | 0.3146 | -938.0 | -738.0 | |
| 0.00 | 0.82 | 0.00 | 0.43 | 14.53 | 166.04 | 13.09 | 315.40 | 0.3135 | -991.0 | -788.1 | |
| 0.00 | 1.63 | 0.00 | 0.85 | 15.16 | 165.82 | 12.87 | 317.30 | 0.3183 | -954.0 | -793.3 | |
| 0.00 | 0.73 | 0.00 | 0.38 | 14.94 | 165.81 | 12.85 | 316.84 | 0.3155 | -878.0 | -705.9 | |
| 0.00 | 1.91 | 0.00 | 1.00 | 16.23 | 165.40 | 12.45 | 320.49 | 0.3267 | 790.0 | 662.4 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 18.26 | 165.38 | 12.42 | 324.37 | 0.3522 | 785.0 | 600.3 | |
| 0.00 | 1.00 | 0.00 | 0.54 | 21.01 | 165.53 | 12.57 | 328.43 | 0.3898 | -753.0 | -566.4 | |
| 0.00 | 1.82 | 0.00 | 0.95 | 17.12 | 165.17 | 12.21 | 322.75 | 0.3354 | 728.0 | 631.7 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 17.18 | 164.91 | 11.96 | 323.44 | 0.3337 | 849.0 | 624.0 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 21.31 | 164.42 | 11.46 | 331.11 | 0.3849 | 707.0 | 612.9 | |
| 0.00 | 2.63 | 0.00 | 1.39 | 18.20 | 164.16 | 11.21 | 326.97 | 0.3401 | 782.0 | 694.6 | |
| 0.00 | 2.99 | 0.00 | 1.57 | 17.50 | 164.12 | 11.16 | 325.86 | 0.3303 | 993.0 | 795.8 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 17.91 | 164.08 | 11.12 | 326.67 | 0.3355 | 997.0 | 836.1 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 18.77 | 164.10 | 11.15 | 328.05 | 0.3474 | 577.0 | 358.8 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 17.31 | 163.88 | 10.92 | 326.08 | 0.3256 | 956.0 | 782.9 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 17.92 | 163.88 | 10.93 | 327.13 | 0.3338 | 899.0 | 807.7 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 18.14 | 163.73 | 10.78 | 327.86 | 0.3355 | 887.0 | 713.8 | |
| 0.00 | 7.17 | 0.00 | 3.74 | 16.84 | 163.59 | 10.63 | 325.92 | 0.3166 | 1080.0 | 832.1 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 17.92 | 163.59 | 10.63 | 327.83 | 0.3312 | 854.0 | 715.4 | |
| 0.00 | 1.91 | 0.00 | 1.00 | 18.43 | 163.36 | 10.40 | 329.22 | 0.3363 | 947.0 | 756.6 | |
| 2.09 | 24.05 | 1.08 | 12.48 | 15.90 | 163.09 | 10.13 | 325.38 | 0.2991 | 1004.0 | 679.5 | |
| 3.54 | -38.00 | 1.84 | -38.00 | 15.71 | 163.04 | 10.09 | 325.12 | 0.2962 | 1069.9 | 999999 | |
| 0.00 | 0.91 | 0.00 | 0.49 | 23.23 | 163.46 | 10.51 | 335.45 | 0.4051 | 768.0 | 619.6 | |
| 6.44 | -38.00 | 3.34 | -38.00 | 15.99 | 162.87 | 9.91 | 326.15 | 0.2984 | 1135.0 | 999999 | |
| 0.00 | 1.72 | 0.00 | 0.90 | 17.45 | 162.39 | 9.44 | 330.02 | 0.3144 | 820.0 | 584.5 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 19.17 | 161.61 | 8.65 | 334.65 | 0.3333 | 724.0 | 573.0 | |
| 4.81 | 6.44 | 2.51 | 3.36 | 18.34 | 161.08 | 8.12 | 334.88 | 0.3173 | 1024.3 | 765.5 | |
| 0.00 | 3.36 | 0.00 | 1.78 | 21.29 | 161.20 | 8.24 | 338.26 | 0.3622 | 801.0 | 717.4 | |
| 0.00 | 3.36 | 0.00 | 1.79 | 21.55 | 161.01 | 8.06 | 338.98 | 0.3650 | 694.0 | 486.0 | |
| 0.00 | 2.36 | 0.00 | 1.22 | 17.39 | 160.48 | 7.53 | 335.15 | 0.2989 | 880.0 | 826.3 | |
| 0.00 | 2.54 | 0.00 | 1.32 | 17.52 | 160.10 | 7.15 | 336.44 | 0.2983 | 1039.0 | 870.9 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 17.71 | 159.89 | 6.93 | 337.34 | 0.2997 | 1135.0 | 1018.4 | |
| 0.00 | 11.98 | 0.00 | 6.23 | 18.00 | 159.83 | 6.88 | 337.88 | 0.3038 | 1110.0 | 879.1 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 17.52 | 159.68 | 6.73 | 337.68 | 0.2956 | 854.0 | 700.2 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 18.41 | 159.69 | 6.73 | 338.82 | 0.3092 | 933.0 | 779.6 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 21.59 | 159.69 | 6.74 | 342.19 | 0.3584 | 712.0 | 599.9 | |
| 0.00 | 1.91 | 0.00 | 0.98 | 16.70 | 159.14 | 6.19 | 338.22 | 0.2795 | 981.0 | 805.6 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 16.89 | 159.02 | 6.07 | 338.86 | 0.2817 | 840.0 | 727.5 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 16.08 | 157.15 | 4.20 | 344.16 | 0.2587 | 836.0 | 607.9 | |
| 0.00 | 1.82 | 0.00 | 0.93 | 14.92 | 156.15 | 3.19 | 346.72 | 0.2354 | 882.0 | 696.8 | |
| 0.00 | 1.91 | 0.00 | 0.97 | 14.83 | 155.92 | 2.97 | 347.53 | 0.2330 | 1040.0 | 799.5 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |