| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.83 | 244.86 | 114.26 | 525.23 | -20.54 | 36.69 | -76.65 | 110.84 | 0.9745 | -33.7 | -133.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.44 | 103.70 | 25.10 | 181.46 | -19.90 | 40.52 | -72.82 | 110.44 | 0.9599 | 558.4 | 118.4 | |
| 2.62 | 122.21 | 5.21 | 296.98 | -21.43 | 38.38 | -74.96 | 111.84 | 0.9696 | 295.9 | -253.5 | |
| 0.00 | 0.63 | 0.00 | 1.19 | -20.60 | 39.30 | -74.03 | 111.06 | 0.9655 | -497.0 | -467.7 | |
| 2.08 | -1.00 | 3.68 | -1.00 | -19.67 | 40.23 | -73.10 | 110.17 | 0.9611 | -295.9 | 999999 | |
| 1.35 | -2.00 | 2.97 | -2.00 | -21.56 | 36.96 | -76.38 | 111.88 | 0.9750 | 110.1 | 999999 | |
| 2.53 | 3.34 | 7.64 | 10.13 | -22.97 | 33.11 | -80.23 | 113.10 | 0.9872 | -293.8 | -189.2 | |
| 0.00 | 8.39 | 0.00 | 21.14 | -22.02 | 35.06 | -78.28 | 112.23 | 0.9815 | -645.0 | -433.0 | |
| 0.00 | 6.59 | 0.00 | 14.33 | -20.36 | 36.92 | -76.41 | 110.64 | 0.9748 | -600.0 | -510.8 | |
| 1.81 | -2.00 | 4.39 | -2.00 | -20.79 | 35.46 | -77.88 | 111.00 | 0.9800 | -570.0 | 999999 | |
| 1.62 | -2.00 | 3.92 | -2.00 | -20.63 | 35.59 | -77.75 | 110.84 | 0.9795 | -504.0 | 999999 | |
| 6.95 | -2.00 | 17.10 | -2.00 | -20.23 | 35.34 | -78.00 | 110.43 | 0.9803 | -397.5 | 999999 | |
| 8.39 | -2.00 | 24.12 | -2.00 | -20.98 | 33.53 | -79.81 | 111.10 | 0.9858 | -407.0 | 999999 | |
| 2.71 | -2.00 | 7.03 | -2.00 | -20.38 | 34.57 | -78.77 | 110.54 | 0.9827 | 309.7 | 999999 | |
| 4.33 | -2.00 | 13.10 | -2.00 | -20.90 | 32.92 | -80.42 | 111.00 | 0.9874 | 317.5 | 999999 | |
| 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. | |