| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61 | 365 | 34 | 203 | -12.37 | 176.36 | -20.26 | 128.56 | 0.4347 | 1125.3 | 364.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 2 | -12.64 | 178.75 | -17.88 | 132.48 | 0.4079 | 676.0 | 495.7 | |
| 0 | 4 | 0 | 2 | -13.25 | 178.54 | -18.09 | 133.25 | 0.4167 | 648.0 | 652.6 | |
| 0 | 4 | 0 | 2 | -11.92 | 178.59 | -18.03 | 130.88 | 0.4023 | 626.0 | 598.9 | |
| 15 | 63 | 8 | 35 | -13.46 | 177.77 | -18.85 | 132.47 | 0.4279 | 1359.4 | 486.2 | |
| 21 | 184 | 12 | 101 | -12.47 | 177.47 | -19.15 | 130.22 | 0.4213 | 1751.0 | 785.0 | |
| 12 | -5 | 7 | -5 | -12.56 | 176.84 | -19.78 | 129.49 | 0.4299 | 1389.6 | 999999 | |
| 7 | -5 | 4 | -5 | -13.12 | 176.79 | -19.83 | 130.44 | 0.4360 | 921.4 | 999999 | |
| 0 | 6 | 0 | 3 | -9.71 | 176.34 | -20.29 | 123.23 | 0.4104 | -527.0 | -481.0 | |
| 0 | 14 | 0 | 8 | -11.74 | 175.86 | -20.77 | 126.63 | 0.4345 | 783.0 | 614.6 | |
| 0 | 5 | 0 | 3 | -12.39 | 175.59 | -21.03 | 127.49 | 0.4437 | 449.0 | 379.3 | |
| 0 | 3 | 0 | 2 | -16.87 | 174.05 | -22.57 | 133.01 | 0.5045 | -476.0 | -429.1 | |
| 0 | 7 | 0 | 4 | -14.96 | 173.98 | -22.65 | 129.91 | 0.4870 | -949.0 | -748.3 | |
| 0 | 8 | 0 | 5 | -9.64 | 174.42 | -22.21 | 120.77 | 0.4356 | -763.0 | -691.5 | |
| 0 | 6 | 0 | 4 | -10.79 | 174.20 | -22.42 | 122.79 | 0.4476 | -853.0 | -618.1 | |
| 0 | 5 | 0 | 3 | -9.02 | 174.00 | -22.63 | 119.06 | 0.4366 | -1036.0 | -833.5 | |
| 3 | 31 | 1 | 17 | -10.77 | 173.48 | -23.14 | 121.94 | 0.4569 | -1215.7 | -640.0 | |
| 3 | 9 | 2 | 5 | -10.90 | 172.79 | -23.84 | 121.45 | 0.4671 | -996.0 | -687.5 | |
| 0 | 3 | 0 | 2 | -11.39 | 172.32 | -24.31 | 121.86 | 0.4771 | -836.0 | -689.7 | |
| 0 | 6 | 0 | 3 | -11.20 | 172.03 | -24.59 | 121.22 | 0.4794 | -467.0 | -342.8 | |
| 0 | 3 | 0 | 2 | -11.89 | 171.58 | -25.05 | 122.00 | 0.4905 | -676.0 | -676.9 | |
| 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. | |