| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.02 | 88.47 | 9.20 | 53.97 | -21.04 | 18.73 | 29.44 | 231.84 | 0.5857 | 445.5 | 366.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.90 | 0.00 | 0.56 | -20.70 | 21.08 | 31.78 | 234.39 | 0.6082 | 492.0 | 484.0 | |
| 0.00 | 2.26 | 0.00 | 1.42 | -22.60 | 20.35 | 31.05 | 231.15 | 0.6138 | 654.0 | 598.8 | |
| 15.02 | 72.37 | 9.20 | 44.34 | -20.53 | 19.63 | 30.34 | 233.49 | 0.5907 | 1190.9 | 485.7 | |
| 0.00 | 1.54 | 0.00 | 0.95 | -22.33 | 19.48 | 30.18 | 230.79 | 0.6024 | 678.0 | 473.9 | |
| 0.00 | 0.72 | 0.00 | 0.44 | -22.04 | 18.88 | 29.58 | 230.70 | 0.5936 | 648.0 | 540.2 | |
| 0.00 | 1.00 | 0.00 | 0.59 | -18.95 | 17.82 | 28.53 | 234.34 | 0.5581 | -575.0 | -390.4 | |
| 0.00 | 0.81 | 0.00 | 0.50 | -24.02 | 16.81 | 27.52 | 226.08 | 0.5881 | 732.0 | 599.7 | |
| 0.00 | 0.90 | 0.00 | 0.55 | -24.22 | 15.59 | 26.29 | 224.60 | 0.5774 | 713.0 | 500.1 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -23.59 | 12.30 | 23.01 | 221.88 | 0.5386 | -773.0 | -621.3 | |
| 0.00 | 0.54 | 0.00 | 0.32 | -23.75 | 12.34 | 23.04 | 221.69 | 0.5406 | -705.0 | -617.7 | |
| 0.00 | 1.63 | 0.00 | 0.95 | -25.15 | 10.25 | 20.95 | 217.33 | 0.5359 | -757.0 | -560.3 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -24.08 | 10.03 | 20.73 | 218.42 | 0.5221 | -824.0 | -730.5 | |
| 0.00 | 2.26 | 0.00 | 1.31 | -25.29 | 8.34 | 19.04 | 214.67 | 0.5207 | -659.0 | -620.5 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -24.85 | 7.81 | 18.51 | 214.47 | 0.5110 | -691.0 | -521.1 | |
| 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. | |