| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.35 | 67.17 | 13.35 | 35.61 | 18.01 | 324.98 | -16.85 | 50.96 | 0.3555 | 197.3 | 276.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 7.14 | 0.00 | 3.74 | 17.79 | 327.09 | -14.74 | 48.06 | 0.3271 | -417.0 | -565.8 | |
| 14.63 | 20.12 | 7.65 | 10.52 | 17.12 | 326.92 | -14.91 | 50.01 | 0.3223 | -1069.2 | -740.0 | |
| 0.00 | 1.13 | 0.00 | 0.59 | 17.08 | 326.50 | -15.32 | 50.85 | 0.3272 | -504.0 | -459.3 | |
| 2.18 | 3.75 | 1.15 | 1.98 | 18.06 | 325.50 | -16.32 | 50.17 | 0.3495 | 849.7 | 799.1 | |
| 0.00 | 1.31 | 0.00 | 0.69 | 16.32 | 325.63 | -16.20 | 54.19 | 0.3316 | 778.0 | 541.8 | |
| 4.01 | 5.75 | 2.13 | 3.05 | 18.10 | 324.71 | -17.12 | 51.32 | 0.3599 | 1075.5 | 628.2 | |
| 0.00 | 1.31 | 0.00 | 0.70 | 18.53 | 324.50 | -17.32 | 50.68 | 0.3665 | 1002.0 | 797.6 | |
| 0.00 | 1.65 | 0.00 | 0.88 | 17.64 | 324.56 | -17.27 | 52.62 | 0.3575 | 899.0 | 576.2 | |
| 3.14 | 13.94 | 1.67 | 7.42 | 18.21 | 324.20 | -17.62 | 51.83 | 0.3673 | 926.6 | 764.5 | |
| 0.00 | 1.13 | 0.00 | 0.61 | 18.28 | 323.21 | -18.62 | 53.11 | 0.3807 | 833.0 | 671.0 | |
| 1.39 | 2.44 | 0.75 | 1.31 | 19.25 | 322.89 | -18.93 | 51.43 | 0.3935 | 980.4 | 930.0 | |
| 0.00 | 1.57 | 0.00 | 0.85 | 19.40 | 322.71 | -19.12 | 51.37 | 0.3971 | 836.0 | 754.2 | |
| 0.00 | 0.96 | 0.00 | 0.52 | 20.57 | 322.56 | -19.27 | 49.20 | 0.4098 | 710.0 | 658.9 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 18.67 | 321.02 | -20.81 | 55.03 | 0.4125 | 671.0 | 537.7 | |
| 0.00 | 0.52 | 0.00 | 0.29 | 19.97 | 319.27 | -22.56 | 54.37 | 0.4454 | 868.0 | 709.2 | |
| 0.00 | 1.74 | 0.00 | 0.98 | 23.00 | 318.55 | -23.27 | 49.61 | 0.4795 | 832.0 | 668.2 | |
| 0.00 | 0.96 | 0.00 | 0.53 | 19.52 | 318.96 | -22.87 | 55.57 | 0.4459 | 778.0 | 598.5 | |
| 0.00 | 0.70 | 0.00 | 0.38 | 15.48 | 317.16 | -24.67 | 65.49 | 0.4439 | 541.0 | 513.0 | |
| 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. | |