| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.26 | 53.02 | 11.68 | 65.32 | 16.74 | 166.38 | 65.82 | 287.35 | 0.9166 | -212.8 | -273.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.45 | 0.00 | 3.39 | 16.34 | 169.30 | 68.75 | 286.67 | 0.9351 | -624.0 | -538.6 | |
| 0.00 | 1.82 | 0.00 | 2.34 | 15.73 | 167.67 | 67.12 | 286.13 | 0.9248 | -215.0 | -223.4 | |
| 6.90 | 10.53 | 8.87 | 13.52 | 16.24 | 167.61 | 67.05 | 286.69 | 0.9246 | -503.3 | -481.3 | |
| 0.00 | 6.81 | 0.00 | 8.71 | 16.75 | 167.39 | 66.84 | 287.26 | 0.9235 | -601.0 | -526.3 | |
| 0.00 | 1.45 | 0.00 | 1.81 | 16.04 | 166.83 | 66.27 | 286.54 | 0.9195 | -518.0 | -480.2 | |
| 0.00 | 1.09 | 0.00 | 1.36 | 16.20 | 166.85 | 66.30 | 286.71 | 0.9197 | -362.0 | -298.2 | |
| 0.00 | 1.63 | 0.00 | 1.98 | 16.01 | 166.02 | 65.46 | 286.57 | 0.9140 | 7.0 | 5.3 | |
| 0.00 | 11.71 | 0.00 | 14.10 | 16.81 | 165.77 | 65.21 | 287.47 | 0.9128 | -425.0 | -378.0 | |
| 0.00 | 0.91 | 0.00 | 1.08 | 16.73 | 165.33 | 64.78 | 287.42 | 0.9098 | 197.0 | 132.8 | |
| 2.36 | 9.81 | 2.81 | 11.75 | 17.20 | 165.42 | 64.86 | 287.94 | 0.9107 | 326.0 | -85.3 | |
| 0.00 | 0.45 | 0.00 | 0.52 | 16.31 | 164.62 | 64.07 | 287.03 | 0.9045 | 267.0 | 258.8 | |
| 0.00 | 2.18 | 0.00 | 2.60 | 17.64 | 165.49 | 64.93 | 288.41 | 0.9115 | 430.0 | 254.3 | |
| 0.00 | 2.18 | 0.00 | 2.16 | 19.12 | 159.52 | 58.96 | 290.87 | 0.8684 | 566.0 | 413.2 | |
| 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. | |