| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.03 | 331.59 | 30.25 | 169.28 | 16.33 | 25.57 | -9.75 | 42.23 | 0.2369 | -46.8 | -144.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.14 | 188.05 | 15.23 | 94.98 | 15.85 | 28.50 | -6.82 | 35.84 | 0.1960 | -1453.6 | -434.7 | |
| 0.00 | 2.70 | 0.00 | 1.37 | 17.97 | 28.01 | -7.31 | 31.88 | 0.2303 | -815.0 | -546.6 | |
| 0.00 | 2.52 | 0.00 | 1.28 | 17.85 | 27.79 | -7.53 | 32.94 | 0.2305 | -807.0 | -677.6 | |
| 0.00 | 1.62 | 0.00 | 0.83 | 18.68 | 27.40 | -7.92 | 32.26 | 0.2457 | -817.0 | -602.9 | |
| 1.35 | 4.68 | 0.68 | 2.37 | 16.36 | 27.40 | -7.92 | 38.34 | 0.2141 | -897.7 | -737.1 | |
| 0.00 | 3.06 | 0.00 | 1.56 | 16.53 | 26.53 | -8.79 | 40.69 | 0.2257 | -994.0 | -760.2 | |
| 0.99 | 10.98 | 0.50 | 5.58 | 16.31 | 26.25 | -9.07 | 42.23 | 0.2261 | -1254.8 | -845.1 | |
| 0.45 | -7.00 | 0.23 | -7.00 | 16.40 | 26.09 | -9.23 | 42.45 | 0.2291 | -1046.0 | 999999 | |
| 0.00 | 6.21 | 0.00 | 3.17 | 16.98 | 26.03 | -9.29 | 40.89 | 0.2370 | -928.0 | -777.7 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 16.86 | 25.78 | -9.54 | 42.00 | 0.2382 | -791.0 | -620.6 | |
| 0.36 | 1.44 | 0.18 | 0.73 | 16.67 | 25.56 | -9.76 | 43.18 | 0.2384 | -924.0 | -823.7 | |
| 0.00 | 1.98 | 0.00 | 1.01 | 16.59 | 24.83 | -10.49 | 45.42 | 0.2462 | -962.0 | -660.2 | |
| 0.00 | 1.71 | 0.00 | 0.87 | 15.94 | 24.47 | -10.85 | 48.35 | 0.2432 | -823.0 | -594.3 | |
| 0.00 | 2.07 | 0.00 | 1.06 | 15.96 | 24.06 | -11.26 | 49.32 | 0.2488 | -965.0 | -772.7 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 15.96 | 23.86 | -11.46 | 49.79 | 0.2512 | -747.0 | -556.5 | |
| 0.00 | 2.97 | 0.00 | 1.55 | 18.92 | 21.14 | -14.18 | 47.36 | 0.3164 | 796.0 | 651.8 | |
| 0.00 | 3.33 | 0.00 | 1.73 | 17.53 | 21.19 | -14.13 | 50.84 | 0.3015 | 863.0 | 710.7 | |
| 0.00 | 7.92 | 0.00 | 4.11 | 16.91 | 21.14 | -14.18 | 52.63 | 0.2962 | 353.0 | 640.3 | |
| 0.00 | 1.53 | 0.00 | 0.79 | 15.92 | 21.05 | -14.27 | 55.64 | 0.2884 | 631.0 | 524.5 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 17.30 | 20.91 | -14.41 | 51.96 | 0.3029 | 1021.0 | 784.3 | |
| 0.90 | 2.88 | 0.47 | 1.49 | 16.16 | 20.90 | -14.42 | 55.19 | 0.2926 | 1223.0 | 975.7 | |
| 1.89 | 6.66 | 0.98 | 3.47 | 17.51 | 20.63 | -14.69 | 51.90 | 0.3086 | 1026.7 | 835.4 | |
| 0.81 | 5.49 | 0.42 | 2.85 | 16.89 | 20.68 | -14.64 | 53.49 | 0.3022 | 1125.4 | 839.8 | |
| 0.00 | 2.97 | 0.00 | 1.54 | 16.00 | 20.72 | -14.60 | 55.97 | 0.2937 | 990.0 | 843.4 | |
| 0.00 | 2.16 | 0.00 | 1.13 | 18.72 | 20.50 | -14.82 | 49.05 | 0.3222 | 829.0 | 659.2 | |
| 0.00 | 2.16 | 0.00 | 1.13 | 18.09 | 20.45 | -14.87 | 50.70 | 0.3166 | 1093.0 | 809.0 | |
| 0.00 | 3.06 | 0.00 | 1.60 | 17.75 | 20.42 | -14.90 | 51.65 | 0.3137 | 880.0 | 729.5 | |
| 0.00 | 2.25 | 0.00 | 1.18 | 19.11 | 20.26 | -15.06 | 48.51 | 0.3291 | 629.0 | 599.5 | |
| 0.00 | 2.25 | 0.00 | 1.17 | 17.01 | 20.41 | -14.91 | 53.64 | 0.3068 | 1068.0 | 819.4 | |
| 0.00 | 5.31 | 0.00 | 2.77 | 17.90 | 20.04 | -15.28 | 51.92 | 0.3200 | 645.0 | 648.0 | |
| 0.90 | 6.84 | 0.47 | 3.57 | 17.22 | 20.03 | -15.29 | 53.73 | 0.3138 | 1186.6 | 815.7 | |
| 0.00 | 2.34 | 0.00 | 1.22 | 16.85 | 20.03 | -15.29 | 54.73 | 0.3105 | 867.0 | 731.7 | |
| 0.00 | 1.62 | 0.00 | 0.85 | 17.58 | 19.70 | -15.61 | 53.31 | 0.3214 | 864.0 | 718.6 | |
| 0.00 | 1.26 | 0.00 | 0.66 | 17.18 | 19.71 | -15.61 | 54.37 | 0.3178 | 809.0 | 720.7 | |
| 13.68 | 22.85 | 7.13 | 11.91 | 16.18 | 19.43 | -15.89 | 57.53 | 0.3131 | 1149.2 | 594.8 | |
| 0.45 | 3.78 | 0.24 | 1.97 | 16.45 | 19.18 | -16.14 | 57.16 | 0.3188 | 971.2 | 716.8 | |
| 7.11 | 11.43 | 3.72 | 5.98 | 16.97 | 19.10 | -16.22 | 55.87 | 0.3242 | 981.7 | 809.0 | |
| 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. | |