| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.46 | 0.00 | 10.82 | 14.55 | 57.44 | 6.31 | 327.28 | 0.1864 | 293.2 | 120.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.88 | 0.00 | 0.45 | 11.41 | 64.29 | 13.16 | 292.87 | 0.2433 | -667.0 | -418.2 | |
| 0.00 | 1.14 | 0.00 | 0.58 | 14.68 | 60.62 | 9.49 | 313.16 | 0.2196 | -792.0 | -608.5 | |
| 0.00 | 3.24 | 0.00 | 1.66 | 18.12 | 60.61 | 9.47 | 323.13 | 0.2619 | -908.0 | -739.8 | |
| 0.00 | 2.63 | 0.00 | 1.35 | 17.70 | 60.20 | 9.07 | 323.28 | 0.2522 | -758.0 | -724.4 | |
| 0.00 | 1.05 | 0.00 | 0.53 | 16.71 | 59.14 | 8.01 | 324.07 | 0.2283 | -772.0 | -678.2 | |
| 0.00 | 1.14 | 0.00 | 0.57 | 12.66 | 58.86 | 7.73 | 311.00 | 0.1747 | 778.0 | 587.6 | |
| 0.00 | 1.40 | 0.00 | 0.70 | 13.06 | 58.25 | 7.12 | 315.02 | 0.1717 | 962.0 | 733.1 | |
| 0.00 | 1.05 | 0.00 | 0.53 | 13.37 | 57.64 | 6.51 | 318.81 | 0.1683 | 769.0 | 624.5 | |
| 0.00 | 1.66 | 0.00 | 0.83 | 13.69 | 55.89 | 4.76 | 328.47 | 0.1548 | 974.0 | 724.4 | |
| 0.00 | 1.66 | 0.00 | 0.83 | 13.28 | 54.65 | 3.52 | 334.31 | 0.1383 | 1038.0 | 886.5 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 12.65 | 54.39 | 3.26 | 333.87 | 0.1266 | 845.0 | 712.4 | |
| 0.00 | 1.49 | 0.00 | 0.74 | 12.95 | 53.84 | 2.71 | 338.72 | 0.1276 | 779.0 | 516.6 | |
| 0.00 | 1.93 | 0.00 | 0.96 | 12.90 | 52.98 | 1.85 | 344.98 | 0.1220 | 994.0 | 772.1 | |
| 0.00 | 1.23 | 0.00 | 0.61 | 11.70 | 50.37 | -0.76 | 7.64 | 0.0978 | 863.0 | 685.9 | |
| 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. | |