| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.22 | 0.00 | 15.19 | -22.95 | 93.63 | -29.77 | 131.66 | 0.6137 | -226.2 | -80.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.11 | 0.00 | 0.66 | -23.96 | 101.26 | -22.14 | 140.83 | 0.5473 | 732.0 | 630.4 | |
| 0.00 | 0.86 | 0.00 | 0.52 | -23.02 | 97.02 | -26.38 | 134.87 | 0.5793 | 744.0 | 644.8 | |
| 0.00 | 1.54 | 0.00 | 0.93 | -22.08 | 96.96 | -26.44 | 133.55 | 0.5714 | 693.0 | 532.0 | |
| 0.00 | 2.05 | 0.00 | 1.28 | -23.72 | 94.93 | -28.47 | 133.77 | 0.6065 | 789.0 | 713.4 | |
| 0.00 | 3.25 | 0.00 | 2.02 | -23.59 | 94.74 | -28.66 | 133.42 | 0.6073 | 713.0 | 651.8 | |
| 0.00 | 0.60 | 0.00 | 0.37 | -22.13 | 95.08 | -28.32 | 131.78 | 0.5915 | -710.0 | -539.6 | |
| 0.00 | 1.54 | 0.00 | 0.93 | -20.21 | 95.09 | -28.31 | 129.10 | 0.5756 | -572.0 | -444.4 | |
| 0.00 | 1.37 | 0.00 | 0.87 | -24.13 | 93.49 | -29.90 | 132.99 | 0.6243 | -656.0 | -437.7 | |
| 0.00 | 0.86 | 0.00 | 0.54 | -23.67 | 93.12 | -30.27 | 132.08 | 0.6244 | -732.0 | -638.2 | |
| 0.00 | 1.11 | 0.00 | 0.71 | -24.33 | 92.72 | -30.67 | 132.59 | 0.6337 | -666.0 | -586.7 | |
| 0.00 | 1.28 | 0.00 | 0.82 | -23.65 | 91.85 | -31.55 | 130.98 | 0.6372 | -722.0 | -543.7 | |
| 0.00 | 0.86 | 0.00 | 0.55 | -23.23 | 91.81 | -31.59 | 130.40 | 0.6344 | -665.0 | -554.2 | |
| 0.00 | 1.45 | 0.00 | 0.91 | -20.43 | 92.28 | -31.12 | 126.98 | 0.6086 | -612.0 | -487.7 | |
| 0.00 | 1.37 | 0.00 | 0.88 | -23.46 | 91.52 | -31.88 | 130.47 | 0.6391 | -563.0 | -441.7 | |
| 0.00 | 1.80 | 0.00 | 1.16 | -23.33 | 91.25 | -32.15 | 130.09 | 0.6409 | -283.0 | -186.3 | |
| 0.00 | 1.37 | 0.00 | 0.85 | -19.33 | 91.45 | -31.95 | 124.77 | 0.6101 | -684.0 | -570.0 | |
| 0.00 | 1.80 | 0.00 | 1.19 | -24.62 | 89.83 | -33.56 | 130.64 | 0.6647 | -651.0 | -552.8 | |
| 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. | |