| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.87 | 86.13 | 2.01 | 45.23 | -18.12 | 141.09 | 9.31 | 206.99 | 0.3281 | 363.1 | 379.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.62 | 0.00 | 0.89 | -20.00 | 149.49 | 17.71 | 222.49 | 0.4249 | 858.0 | 652.6 | |
| 0.00 | 1.71 | 0.00 | 0.93 | -19.65 | 149.35 | 17.57 | 222.87 | 0.4196 | 843.0 | 723.5 | |
| 0.00 | 0.90 | 0.00 | 0.48 | -16.06 | 148.59 | 16.81 | 228.51 | 0.3726 | 658.0 | 583.2 | |
| 0.00 | 1.71 | 0.00 | 0.91 | -16.03 | 148.30 | 16.51 | 228.08 | 0.3687 | 880.0 | 695.3 | |
| 0.00 | 2.70 | 0.00 | 1.47 | -19.69 | 148.61 | 16.83 | 221.63 | 0.4121 | 770.0 | 694.8 | |
| 0.00 | 2.52 | 0.00 | 1.34 | -16.07 | 148.07 | 16.29 | 227.63 | 0.3663 | 814.0 | 709.6 | |
| 0.00 | 0.27 | 0.00 | 0.14 | -15.29 | 147.38 | 15.60 | 228.13 | 0.3499 | 69.0 | 70.7 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -19.41 | 147.68 | 15.89 | 220.55 | 0.3990 | 908.0 | 788.9 | |
| 0.00 | 1.26 | 0.00 | 0.68 | -19.06 | 147.58 | 15.79 | 220.98 | 0.3939 | 808.0 | 498.1 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -19.42 | 147.28 | 15.49 | 219.84 | 0.3949 | 823.0 | 672.2 | |
| 0.00 | 2.07 | 0.00 | 1.10 | -16.83 | 147.01 | 15.23 | 224.21 | 0.3622 | 811.0 | 709.3 | |
| 0.00 | 1.62 | 0.00 | 0.88 | -20.69 | 147.34 | 15.56 | 217.83 | 0.4108 | 590.0 | 510.8 | |
| 0.00 | 0.72 | 0.00 | 0.38 | -15.33 | 146.64 | 14.85 | 226.69 | 0.3412 | 784.0 | 595.8 | |
| 0.00 | 0.99 | 0.00 | 0.53 | -19.20 | 146.82 | 15.04 | 219.41 | 0.3876 | 955.0 | 804.5 | |
| 0.00 | 1.98 | 0.00 | 1.07 | -20.28 | 146.89 | 15.11 | 217.71 | 0.4014 | 801.0 | 690.7 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -18.82 | 146.72 | 14.94 | 219.90 | 0.3820 | 842.0 | 706.6 | |
| 0.00 | 1.17 | 0.00 | 0.63 | -20.86 | 146.61 | 14.83 | 216.29 | 0.4058 | 630.0 | 704.5 | |
| 0.00 | 0.36 | 0.00 | 0.19 | -16.83 | 146.03 | 14.25 | 222.35 | 0.3512 | -6.0 | 1.8 | |
| 0.00 | 1.44 | 0.00 | 0.77 | -18.16 | 145.84 | 14.06 | 219.43 | 0.3650 | 704.0 | 559.4 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -17.21 | 145.54 | 13.75 | 220.61 | 0.3504 | 5.0 | 8.8 | |
| 0.00 | 1.35 | 0.00 | 0.72 | -18.41 | 145.50 | 13.71 | 218.29 | 0.3646 | 997.0 | 850.1 | |
| 0.00 | 0.81 | 0.00 | 0.43 | -18.00 | 145.43 | 13.65 | 218.91 | 0.3589 | 887.0 | 739.6 | |
| 0.00 | 1.53 | 0.00 | 0.81 | -18.73 | 145.39 | 13.61 | 217.52 | 0.3675 | 718.0 | 573.3 | |
| 0.54 | 1.89 | 0.29 | 1.01 | -19.46 | 145.42 | 13.64 | 216.32 | 0.3769 | 902.5 | 730.9 | |
| 0.00 | 1.35 | 0.00 | 0.71 | -18.42 | 143.96 | 12.17 | 215.08 | 0.3496 | 26.0 | 14.5 | |
| 0.00 | 2.34 | 0.00 | 1.23 | -18.62 | 142.30 | 10.52 | 211.00 | 0.3375 | 582.0 | 613.8 | |
| 0.00 | 1.98 | 0.00 | 1.03 | -15.85 | 141.89 | 10.11 | 214.97 | 0.2959 | 869.0 | 676.8 | |
| 0.00 | 1.26 | 0.00 | 0.65 | -17.59 | 138.86 | 7.08 | 203.48 | 0.2962 | -800.0 | -644.1 | |
| 0.00 | 1.62 | 0.00 | 0.84 | -17.88 | 137.40 | 5.61 | 198.69 | 0.2918 | -839.0 | -598.6 | |
| 0.72 | 37.35 | 0.37 | 19.34 | -18.10 | 136.60 | 4.82 | 195.98 | 0.2914 | -499.9 | 386.3 | |
| 2.61 | -30.00 | 1.35 | -30.00 | -17.85 | 136.37 | 4.59 | 195.50 | 0.2863 | -298.9 | 999999 | |
| 0.00 | 2.88 | 0.00 | 1.49 | -17.44 | 136.36 | 4.58 | 195.88 | 0.2796 | -956.0 | -822.3 | |
| 0.00 | 1.17 | 0.00 | 0.60 | -17.19 | 136.04 | 4.26 | 195.06 | 0.2741 | -904.0 | -720.0 | |
| 0.00 | 1.35 | 0.00 | 0.70 | -17.53 | 135.95 | 4.17 | 194.43 | 0.2794 | -708.0 | -584.3 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -17.41 | 135.85 | 4.07 | 194.22 | 0.2769 | -859.0 | -713.3 | |
| 0.00 | 0.99 | 0.00 | 0.51 | -18.32 | 135.81 | 4.03 | 193.27 | 0.2916 | 801.0 | 579.9 | |
| 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. | |