| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.63 | 28.87 | 1.84 | 14.81 | 15.11 | 24.43 | -7.74 | 31.44 | 0.2521 | -148.4 | -328.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.73 | 0.00 | 0.38 | 19.35 | 26.35 | -5.82 | 18.51 | 0.3025 | -828.0 | -626.6 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 15.57 | 25.58 | -6.59 | 26.48 | 0.2489 | -946.0 | -809.7 | |
| 3.63 | 4.18 | 1.84 | 2.12 | 13.14 | 25.62 | -6.55 | 31.63 | 0.2127 | 983.0 | 939.7 | |
| 0.00 | 2.91 | 0.00 | 1.49 | 15.66 | 25.39 | -6.78 | 26.98 | 0.2518 | -878.0 | -643.0 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 10.12 | 25.32 | -6.85 | 42.49 | 0.1746 | -900.0 | -691.7 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 15.47 | 24.95 | -7.22 | 28.82 | 0.2525 | -884.0 | -774.1 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 13.35 | 24.92 | -7.25 | 33.70 | 0.2222 | 692.0 | 461.7 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 13.38 | 24.67 | -7.50 | 34.53 | 0.2251 | 651.0 | 542.5 | |
| 0.00 | 2.54 | 0.00 | 1.30 | 15.72 | 24.33 | -7.84 | 30.32 | 0.2612 | -963.0 | -724.4 | |
| 0.00 | 3.63 | 0.00 | 1.87 | 16.12 | 24.06 | -8.11 | 30.36 | 0.2693 | -786.0 | -811.1 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 14.62 | 24.03 | -8.15 | 33.66 | 0.2484 | -664.0 | -386.9 | |
| 0.00 | 1.63 | 0.00 | 0.83 | 14.09 | 23.82 | -8.35 | 35.59 | 0.2431 | 829.0 | 579.1 | |
| 0.00 | 2.36 | 0.00 | 1.22 | 16.15 | 23.74 | -8.43 | 31.27 | 0.2725 | -778.0 | -598.7 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 17.44 | 23.20 | -8.97 | 30.39 | 0.2954 | -561.0 | -438.2 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 16.77 | 22.23 | -9.94 | 34.27 | 0.2948 | 840.0 | 545.9 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 17.20 | 21.10 | -11.07 | 36.26 | 0.3114 | 868.0 | 767.8 | |
| 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. | |