| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.32 | 45.12 | 6.98 | 25.49 | 16.18 | 279.44 | 26.64 | 295.97 | 0.4804 | -262.5 | -227.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.87 | 0.00 | 0.53 | 12.14 | 288.76 | 35.97 | 284.01 | 0.5941 | -635.0 | -552.8 | |
| 0.00 | 0.87 | 0.00 | 0.52 | 12.43 | 287.16 | 34.37 | 284.92 | 0.5728 | -656.0 | -535.1 | |
| 0.00 | 1.13 | 0.00 | 0.67 | 15.87 | 285.56 | 32.77 | 291.46 | 0.5616 | -644.0 | -601.2 | |
| 0.00 | 2.95 | 0.00 | 1.76 | 15.60 | 285.47 | 32.68 | 291.03 | 0.5594 | -321.0 | -438.1 | |
| 0.00 | 1.21 | 0.00 | 0.71 | 14.04 | 283.62 | 30.83 | 289.07 | 0.5281 | -710.0 | -532.7 | |
| 0.00 | 1.48 | 0.00 | 0.85 | 18.30 | 280.75 | 27.96 | 298.59 | 0.5090 | -847.0 | -749.5 | |
| 12.32 | 19.70 | 6.98 | 11.16 | 16.21 | 280.02 | 27.23 | 295.19 | 0.4875 | -931.0 | -713.4 | |
| 0.00 | 1.56 | 0.00 | 0.88 | 18.05 | 279.12 | 26.33 | 299.37 | 0.4859 | -731.0 | -537.7 | |
| 0.00 | 3.12 | 0.00 | 1.76 | 17.75 | 278.90 | 26.11 | 298.98 | 0.4811 | -738.0 | -641.5 | |
| 0.00 | 1.65 | 0.00 | 0.93 | 17.43 | 278.36 | 25.57 | 298.80 | 0.4719 | -286.0 | -235.1 | |
| 0.00 | 1.48 | 0.00 | 0.80 | 12.23 | 276.21 | 23.41 | 289.29 | 0.4132 | 724.0 | 571.2 | |
| 0.00 | 0.69 | 0.00 | 0.38 | 17.35 | 276.36 | 23.57 | 300.39 | 0.4443 | 725.0 | 538.0 | |
| 0.00 | 0.78 | 0.00 | 0.43 | 16.65 | 276.13 | 23.34 | 299.17 | 0.4365 | 797.0 | 588.8 | |
| 0.00 | 1.82 | 0.00 | 0.99 | 13.10 | 275.49 | 22.70 | 291.82 | 0.4066 | 743.0 | 626.7 | |
| 0.00 | 1.21 | 0.00 | 0.65 | 13.52 | 274.64 | 21.85 | 293.49 | 0.3962 | 581.0 | 560.5 | |
| 0.00 | 1.48 | 0.00 | 0.82 | 22.31 | 274.91 | 22.12 | 311.34 | 0.4659 | 685.0 | 553.4 | |
| 0.00 | 0.78 | 0.00 | 0.41 | 16.23 | 270.64 | 17.84 | 304.46 | 0.3584 | 795.0 | 634.7 | |
| 0.00 | 2.34 | 0.00 | 1.24 | 17.27 | 269.30 | 16.51 | 308.92 | 0.3503 | 721.0 | 587.8 | |
| 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. | |