| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 91.33 | 281.57 | 46.45 | 143.30 | -4.85 | 86.65 | 9.61 | 226.85 | 0.2287 | 70.7 | 87.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.04 | 0.00 | 0.54 | -8.50 | 91.63 | 14.59 | 229.47 | 0.3292 | 768.0 | 686.2 | |
| 0.00 | 1.73 | 0.00 | 0.89 | -5.07 | 90.94 | 13.90 | 237.17 | 0.2861 | 618.0 | 569.7 | |
| 0.00 | 5.10 | 0.00 | 2.63 | -5.03 | 90.36 | 13.32 | 236.16 | 0.2775 | 861.0 | 755.6 | |
| 10.63 | 22.38 | 5.46 | 11.50 | -4.31 | 90.32 | 13.27 | 238.30 | 0.2703 | 1029.5 | 684.3 | |
| 3.97 | 42.51 | 2.04 | 21.77 | -4.11 | 89.70 | 12.66 | 237.68 | 0.2598 | 1035.9 | 598.8 | |
| 3.89 | -5.00 | 1.99 | -5.00 | -3.90 | 89.64 | 12.59 | 238.25 | 0.2570 | 1095.8 | 999999 | |
| 11.75 | -5.00 | 6.02 | -5.00 | -4.11 | 89.37 | 12.32 | 237.00 | 0.2550 | 1186.7 | 999999 | |
| 0.00 | 1.47 | 0.00 | 0.76 | -6.06 | 89.34 | 12.30 | 230.92 | 0.2741 | 937.0 | 829.1 | |
| 0.60 | 1.64 | 0.31 | 0.84 | -3.74 | 89.03 | 11.98 | 237.49 | 0.2468 | 1018.7 | 830.2 | |
| 1.12 | 5.27 | 0.57 | 2.70 | -4.58 | 88.95 | 11.90 | 234.52 | 0.2536 | 1021.1 | 875.1 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -0.27 | 88.82 | 11.78 | 250.61 | 0.2174 | 851.0 | 690.9 | |
| 0.00 | 0.86 | 0.00 | 0.44 | -3.98 | 88.69 | 11.65 | 235.95 | 0.2443 | 821.0 | 619.0 | |
| 0.00 | 1.30 | 0.00 | 0.66 | -4.99 | 88.31 | 11.27 | 231.69 | 0.2492 | 819.0 | 691.7 | |
| 0.00 | 6.39 | 0.00 | 3.28 | -6.02 | 88.15 | 11.11 | 228.18 | 0.2582 | 703.0 | 809.1 | |
| 0.00 | 1.81 | 0.00 | 0.93 | -5.68 | 88.05 | 11.01 | 228.91 | 0.2533 | 933.0 | 729.3 | |
| 0.00 | 4.41 | 0.00 | 2.25 | -4.84 | 87.92 | 10.87 | 231.19 | 0.2423 | 1101.0 | 846.2 | |
| 0.00 | 1.56 | 0.00 | 0.79 | -5.41 | 87.68 | 10.64 | 228.78 | 0.2455 | 1097.0 | 979.9 | |
| 0.00 | 0.69 | 0.00 | 0.35 | -5.92 | 87.69 | 10.65 | 227.26 | 0.2514 | 761.0 | 657.6 | |
| 0.00 | 4.92 | 0.00 | 2.51 | -4.50 | 87.43 | 10.38 | 231.00 | 0.2322 | -732.0 | -703.6 | |
| 3.46 | 30.07 | 1.75 | 15.25 | -3.87 | 87.05 | 10.01 | 232.19 | 0.2205 | 956.5 | 848.2 | |
| 0.00 | 1.12 | 0.00 | 0.57 | -5.55 | 86.99 | 9.94 | 226.41 | 0.2384 | -654.0 | -482.2 | |
| 5.01 | -20.00 | 2.54 | -20.00 | -3.71 | 86.84 | 9.80 | 232.15 | 0.2161 | 1305.4 | 999999 | |
| 0.95 | -20.00 | 0.48 | -20.00 | -3.74 | 86.57 | 9.53 | 231.26 | 0.2127 | 1184.9 | 999999 | |
| 0.00 | 3.71 | 0.00 | 1.89 | -5.63 | 86.59 | 9.55 | 224.99 | 0.2346 | -811.0 | -707.9 | |
| 0.00 | 1.30 | 0.00 | 0.66 | -5.51 | 86.35 | 9.31 | 224.63 | 0.2302 | -784.0 | -673.5 | |
| 0.00 | 3.71 | 0.00 | 1.89 | -5.68 | 85.81 | 8.77 | 222.38 | 0.2260 | -803.0 | -739.6 | |
| 2.76 | 131.49 | 1.41 | 66.62 | -5.89 | 85.54 | 8.50 | 220.88 | 0.2256 | -910.7 | -467.1 | |
| 4.67 | -27.00 | 2.37 | -27.00 | -5.80 | 85.30 | 8.25 | 220.33 | 0.2217 | -1058.3 | 999999 | |
| 0.00 | 1.47 | 0.00 | 0.74 | -4.17 | 85.04 | 7.99 | 224.68 | 0.1982 | 931.0 | 732.0 | |
| 7.52 | -27.00 | 3.81 | -27.00 | -5.52 | 84.81 | 7.77 | 219.44 | 0.2128 | -1182.3 | 999999 | |
| 1.99 | -27.00 | 1.01 | -27.00 | -4.89 | 84.74 | 7.70 | 221.17 | 0.2037 | -470.3 | 999999 | |
| 26.44 | -27.00 | 13.37 | -27.00 | -5.04 | 84.50 | 7.46 | 219.80 | 0.2030 | -1100.9 | 999999 | |
| 6.57 | -27.00 | 3.32 | -27.00 | -5.37 | 84.27 | 7.22 | 217.87 | 0.2049 | -1155.9 | 999999 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -5.12 | 83.57 | 6.53 | 215.84 | 0.1943 | 716.0 | 557.1 | |
| 0.00 | 2.16 | 0.00 | 1.09 | -7.42 | 80.62 | 3.58 | 197.47 | 0.2071 | -727.0 | -641.8 | |
| 0.00 | 1.04 | 0.00 | 0.53 | -9.26 | 77.20 | 0.16 | 180.68 | 0.2293 | -886.0 | -720.2 | |
| 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. | |