| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.42 | 0.00 | 11.63 | 14.38 | 15.02 | -7.33 | 23.29 | 0.2785 | -483.7 | -351.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.13 | 0.00 | 1.08 | 12.38 | 21.46 | -0.90 | 4.13 | 0.2130 | -792.0 | -719.6 | |
| 0.00 | 1.53 | 0.00 | 0.77 | 8.54 | 21.41 | -0.95 | 6.42 | 0.1471 | -936.0 | -729.7 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 8.00 | 20.16 | -2.20 | 15.59 | 0.1422 | -838.0 | -626.6 | |
| 0.00 | 0.94 | 0.00 | 0.48 | 13.29 | 19.46 | -2.90 | 12.24 | 0.2333 | -903.0 | -720.9 | |
| 0.00 | 2.13 | 0.00 | 1.08 | 10.21 | 18.16 | -4.19 | 22.42 | 0.1896 | -997.0 | -775.1 | |
| 0.00 | 1.62 | 0.00 | 0.82 | 12.26 | 16.92 | -5.43 | 23.83 | 0.2301 | -915.0 | -684.8 | |
| 0.00 | 1.71 | 0.00 | 0.87 | 12.11 | 16.92 | -5.43 | 24.10 | 0.2277 | -729.0 | -643.0 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 15.51 | 16.23 | -6.12 | 21.22 | 0.2852 | -689.0 | -525.4 | |
| 0.00 | 1.79 | 0.00 | 0.92 | 13.75 | 15.97 | -6.38 | 24.70 | 0.2596 | -706.0 | -566.9 | |
| 0.00 | 0.60 | 0.00 | 0.31 | 13.81 | 13.92 | -8.44 | 31.14 | 0.2768 | -697.0 | -565.1 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 15.67 | 13.47 | -8.88 | 29.08 | 0.3073 | -794.0 | -631.7 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 17.67 | 12.47 | -9.88 | 28.53 | 0.3440 | -649.0 | -503.9 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 18.61 | 9.14 | -13.21 | 34.40 | 0.3851 | 931.0 | 704.8 | |
| 0.00 | 1.79 | 0.00 | 0.97 | 19.67 | 8.93 | -13.43 | 33.22 | 0.4009 | 794.0 | 575.6 | |
| 0.00 | 2.13 | 0.00 | 1.19 | 21.73 | 4.41 | -17.94 | 37.90 | 0.4678 | 664.0 | 456.8 | |
| 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. | |