| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.78 | 67.45 | 21.09 | 49.02 | -13.26 | 224.87 | -44.60 | 110.84 | 0.7330 | -260.1 | 23.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.55 | 0.00 | 1.05 | -13.31 | 228.86 | -40.62 | 112.48 | 0.6879 | 613.0 | 512.6 | |
| 0.00 | 1.98 | 0.00 | 1.34 | -13.06 | 228.79 | -40.69 | 112.11 | 0.6878 | 618.0 | 525.0 | |
| 2.06 | 11.00 | 1.41 | 7.53 | -12.83 | 228.43 | -41.04 | 111.62 | 0.6911 | 831.6 | 514.5 | |
| 3.09 | -3.00 | 2.12 | -3.00 | -12.95 | 228.28 | -41.19 | 111.74 | 0.6933 | 676.3 | 999999 | |
| 0.00 | 1.63 | 0.00 | 1.13 | -12.87 | 227.81 | -41.66 | 111.43 | 0.6985 | 477.0 | 351.5 | |
| 0.00 | 0.34 | 0.00 | 0.25 | -14.86 | 226.32 | -43.15 | 113.46 | 0.7230 | -672.0 | -673.5 | |
| 7.73 | 9.97 | 5.57 | 7.18 | -15.28 | 226.00 | -43.47 | 113.87 | 0.7281 | -742.7 | -430.0 | |
| 0.95 | 8.85 | 0.67 | 6.30 | -12.50 | 225.82 | -43.66 | 110.13 | 0.7202 | 829.9 | 633.9 | |
| 1.98 | 3.52 | 1.42 | 2.53 | -12.70 | 225.35 | -44.12 | 110.22 | 0.7261 | 612.2 | 471.4 | |
| 0.00 | 1.89 | 0.00 | 1.39 | -12.81 | 223.99 | -45.48 | 109.87 | 0.7416 | -851.0 | -745.5 | |
| 2.32 | 7.47 | 1.74 | 5.61 | -13.39 | 223.06 | -46.41 | 110.29 | 0.7536 | -768.4 | -560.6 | |
| 0.00 | 0.69 | 0.00 | 0.52 | -13.03 | 222.84 | -46.63 | 109.75 | 0.7549 | -544.0 | -436.6 | |
| 0.00 | 0.69 | 0.00 | 0.52 | -12.85 | 222.48 | -46.99 | 109.41 | 0.7582 | -537.0 | -459.0 | |
| 10.65 | 17.87 | 8.16 | 13.67 | -12.90 | 221.88 | -47.59 | 109.28 | 0.7648 | -608.8 | -470.2 | |
| 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. | |