| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.64 | 39.87 | 3.48 | 20.95 | 7.47 | 252.17 | 19.10 | 282.46 | 0.3339 | 558.1 | 430.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.91 | 0.00 | 0.49 | 6.41 | 255.64 | 22.57 | 278.13 | 0.3870 | -775.0 | -649.4 | |
| 0.64 | 1.63 | 0.34 | 0.87 | 7.33 | 254.07 | 21.00 | 281.14 | 0.3638 | -979.7 | -857.5 | |
| 0.00 | 5.27 | 0.00 | 2.79 | 6.97 | 253.52 | 20.45 | 280.39 | 0.3542 | -538.0 | -712.6 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 7.86 | 253.37 | 20.30 | 282.95 | 0.3542 | 767.0 | 511.7 | |
| 1.00 | 8.08 | 0.53 | 4.25 | 8.13 | 252.47 | 19.40 | 284.21 | 0.3406 | 851.9 | 724.9 | |
| 0.73 | -5.00 | 0.38 | -5.00 | 8.04 | 252.33 | 19.26 | 284.04 | 0.3382 | 931.1 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 7.37 | 252.23 | 19.17 | 282.13 | 0.3345 | 826.0 | 680.7 | |
| 0.00 | 2.36 | 0.00 | 1.24 | 7.83 | 251.96 | 18.89 | 283.66 | 0.3316 | 901.0 | 714.8 | |
| 0.00 | 3.09 | 0.00 | 1.62 | 8.60 | 252.00 | 18.93 | 285.88 | 0.3350 | 702.0 | 767.9 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 8.11 | 251.88 | 18.81 | 284.53 | 0.3312 | 1029.0 | 906.6 | |
| 0.00 | 2.54 | 0.00 | 1.33 | 7.29 | 251.58 | 18.51 | 282.25 | 0.3237 | 712.0 | 685.6 | |
| 4.27 | 8.54 | 2.23 | 4.46 | 7.24 | 251.26 | 18.19 | 282.27 | 0.3182 | 1127.0 | 837.0 | |
| 0.00 | 1.73 | 0.00 | 0.90 | 6.34 | 250.51 | 17.44 | 279.79 | 0.3036 | 1091.0 | 879.8 | |
| 0.00 | 1.82 | 0.00 | 0.94 | 6.19 | 250.41 | 17.34 | 279.34 | 0.3016 | 988.0 | 749.0 | |
| 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. | |