| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.97 | 43.02 | 9.70 | 24.30 | -19.66 | 51.07 | 21.90 | 227.01 | 0.4807 | 343.8 | -74.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.26 | 0.00 | 0.73 | -20.08 | 54.58 | 25.41 | 230.79 | 0.5221 | 615.0 | 533.7 | |
| 0.00 | 1.44 | 0.00 | 0.83 | -18.83 | 54.06 | 24.88 | 232.28 | 0.5055 | 681.0 | 600.1 | |
| 14.89 | 21.21 | 8.55 | 12.18 | -19.38 | 53.89 | 24.72 | 231.21 | 0.5081 | 959.3 | 544.5 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -18.64 | 53.64 | 24.46 | 232.16 | 0.4989 | 811.0 | 680.1 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -18.94 | 52.00 | 22.82 | 229.84 | 0.4820 | 759.0 | 576.5 | |
| 0.00 | 1.08 | 0.00 | 0.60 | -15.78 | 50.50 | 21.33 | 233.76 | 0.4357 | 701.0 | 565.5 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -20.52 | 50.69 | 21.52 | 225.68 | 0.4822 | 600.0 | 651.8 | |
| 0.00 | 3.34 | 0.00 | 1.85 | -19.59 | 48.74 | 19.56 | 224.58 | 0.4513 | -916.0 | -827.2 | |
| 2.08 | 5.23 | 1.15 | 2.90 | -19.85 | 48.53 | 19.35 | 223.86 | 0.4517 | -937.4 | -783.0 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -19.86 | 45.95 | 16.77 | 219.93 | 0.4246 | -834.0 | -644.0 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -21.87 | 42.68 | 13.51 | 211.26 | 0.4195 | -805.0 | -679.6 | |
| 0.00 | 3.70 | 0.00 | 2.01 | -21.74 | 42.33 | 13.16 | 210.78 | 0.4149 | -831.0 | -723.4 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -21.55 | 41.84 | 12.67 | 210.11 | 0.4083 | -789.0 | -608.4 | |
| 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. | |