| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.05 | 106.02 | 9.10 | 56.53 | 19.83 | 97.83 | 17.08 | 311.49 | 0.3704 | -269.8 | -298.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.84 | 57.77 | 0.98 | 30.88 | 19.42 | 98.95 | 18.20 | 308.82 | 0.3798 | -1195.6 | -632.6 | |
| 5.77 | 8.04 | 3.10 | 4.32 | 20.10 | 99.03 | 18.28 | 310.15 | 0.3871 | -860.0 | -429.6 | |
| 1.31 | -1.00 | 0.70 | -1.00 | 19.27 | 98.77 | 18.02 | 308.76 | 0.3761 | -1152.5 | 999999 | |
| 0.35 | -1.00 | 0.19 | -1.00 | 19.49 | 98.76 | 18.01 | 309.24 | 0.3780 | -1366.5 | 999999 | |
| 0.79 | -1.00 | 0.42 | -1.00 | 19.37 | 98.45 | 17.70 | 309.45 | 0.3730 | -1012.2 | 999999 | |
| 0.00 | 4.46 | 0.00 | 2.38 | 20.05 | 98.42 | 17.68 | 310.95 | 0.3793 | -894.0 | -746.8 | |
| 0.00 | 1.31 | 0.00 | 0.70 | 19.60 | 98.17 | 17.42 | 310.35 | 0.3718 | -1034.0 | -817.3 | |
| 0.00 | 2.01 | 0.00 | 1.07 | 19.36 | 97.94 | 17.20 | 310.17 | 0.3667 | -924.0 | -654.5 | |
| 0.00 | 2.27 | 0.00 | 1.20 | 19.17 | 96.83 | 16.09 | 311.53 | 0.3512 | -845.0 | -704.1 | |
| 4.81 | 20.63 | 2.55 | 10.95 | 20.93 | 95.99 | 15.24 | 316.75 | 0.3600 | 1104.8 | 696.2 | |
| 2.18 | 2.62 | 1.16 | 1.39 | 20.50 | 95.81 | 15.07 | 316.18 | 0.3532 | 1032.5 | 867.3 | |
| 0.00 | 1.40 | 0.00 | 0.74 | 19.30 | 95.47 | 14.72 | 314.22 | 0.3361 | 644.0 | 408.1 | |
| 0.00 | 4.37 | 0.00 | 2.30 | 19.93 | 95.07 | 14.32 | 316.36 | 0.3384 | 1011.0 | 696.8 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 20.49 | 93.41 | 12.67 | 320.89 | 0.3271 | 851.0 | 697.6 | |
| 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. | |