| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.30 | 160.82 | 40.17 | 179.54 | 11.27 | 10.37 | 61.17 | 286.42 | 0.8972 | -121.6 | -146.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.02 | 85.97 | 17.57 | 100.12 | 11.72 | 11.68 | 62.48 | 286.56 | 0.9077 | -501.6 | -254.2 | |
| 2.34 | -1.00 | 2.67 | -1.00 | 11.46 | 10.98 | 61.78 | 286.45 | 0.9023 | -738.6 | 999999 | |
| 0.00 | 1.22 | 0.00 | 1.40 | 12.21 | 11.02 | 61.82 | 287.25 | 0.9039 | -345.0 | -310.2 | |
| 1.48 | 66.34 | 1.63 | 70.39 | 11.60 | 10.08 | 60.88 | 286.85 | 0.8960 | -544.8 | -1.2 | |
| 0.00 | 1.56 | 0.00 | 1.70 | 10.79 | 9.72 | 60.52 | 286.06 | 0.8918 | -275.0 | -212.8 | |
| 0.69 | 1.74 | 0.75 | 1.86 | 10.32 | 9.44 | 60.24 | 285.62 | 0.8888 | 198.1 | 142.8 | |
| 2.78 | -4.00 | 3.01 | -4.00 | 11.47 | 9.47 | 60.27 | 286.87 | 0.8912 | -632.5 | 999999 | |
| 2.17 | -4.00 | 2.29 | -4.00 | 10.44 | 8.87 | 59.67 | 285.91 | 0.8846 | 451.5 | 999999 | |
| 0.00 | 0.69 | 0.00 | 0.72 | 9.85 | 8.57 | 59.37 | 285.34 | 0.8811 | 283.0 | 292.1 | |
| 1.65 | -4.00 | 1.74 | -4.00 | 10.87 | 8.77 | 59.57 | 286.40 | 0.8846 | 254.5 | 999999 | |
| 6.17 | -4.00 | 6.39 | -4.00 | 10.24 | 8.39 | 59.19 | 285.81 | 0.8804 | 742.4 | 999999 | |
| 2.87 | -4.00 | 2.98 | -4.00 | 10.63 | 8.33 | 59.13 | 286.26 | 0.8807 | 682.3 | 999999 | |
| 0.52 | 1.74 | 0.54 | 1.80 | 11.53 | 8.04 | 58.84 | 287.34 | 0.8803 | 207.3 | 136.4 | |
| 0.61 | 1.56 | 0.60 | 1.55 | 11.17 | 6.76 | 57.56 | 287.31 | 0.8692 | 250.7 | 269.5 | |
| 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. | |