| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.91 | 347.73 | 32.84 | 197.28 | -16.18 | 12.09 | 27.26 | 244.67 | 0.4886 | 874.1 | 403.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.66 | 200.60 | 14.11 | 114.83 | -16.52 | 12.95 | 28.12 | 244.62 | 0.5022 | 1140.1 | 379.9 | |
| 3.66 | -1.00 | 2.08 | -1.00 | -16.50 | 12.60 | 27.77 | 244.42 | 0.4973 | 1324.5 | 999999 | |
| 1.70 | -1.00 | 0.97 | -1.00 | -16.63 | 12.45 | 27.61 | 244.07 | 0.4958 | 1172.8 | 999999 | |
| 0.00 | 3.83 | 0.00 | 2.16 | -15.20 | 12.00 | 27.16 | 246.54 | 0.4822 | 30.0 | -85.5 | |
| 0.00 | 0.85 | 0.00 | 0.48 | -16.63 | 11.55 | 26.71 | 243.43 | 0.4835 | 628.0 | 489.7 | |
| 27.89 | 129.59 | 15.68 | 72.76 | -15.67 | 11.31 | 26.47 | 245.14 | 0.4750 | 1250.8 | 507.0 | |
| 0.00 | 4.68 | 0.00 | 2.62 | -14.81 | 11.09 | 26.25 | 246.73 | 0.4675 | 1045.0 | 876.1 | |
| 0.00 | 1.11 | 0.00 | 0.63 | -18.94 | 11.47 | 26.63 | 239.03 | 0.4965 | 774.0 | 608.5 | |
| 0.00 | 1.19 | 0.00 | 0.65 | -15.20 | 7.18 | 22.34 | 242.81 | 0.4142 | -603.0 | -589.4 | |
| 0.00 | 0.60 | 0.00 | 0.32 | -13.75 | 5.62 | 20.79 | 244.73 | 0.3829 | -807.0 | -693.9 | |
| 0.00 | 0.94 | 0.00 | 0.51 | -18.14 | 5.77 | 20.93 | 234.99 | 0.4163 | -757.0 | -523.8 | |
| 0.00 | 1.36 | 0.00 | 0.74 | -19.06 | 4.39 | 19.55 | 231.38 | 0.4067 | -809.0 | -667.5 | |
| 0.00 | 1.70 | 0.00 | 0.90 | -12.31 | 3.41 | 18.58 | 246.26 | 0.3416 | -790.0 | -592.5 | |
| 0.00 | 1.28 | 0.00 | 0.68 | -19.63 | 1.00 | 16.17 | 225.15 | 0.3716 | -856.0 | -788.1 | |
| 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. | |