| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 82.31 | 445.35 | 90.23 | 488.97 | 15.49 | 60.53 | -63.80 | 75.95 | 0.8913 | -66.8 | 1.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.71 | 0.00 | 1.76 | 20.29 | 62.51 | -61.82 | 70.52 | 0.8789 | -490.0 | -411.5 | |
| 24.23 | 196.80 | 23.24 | 190.52 | 15.90 | 64.82 | -59.52 | 75.46 | 0.8582 | -917.1 | -201.8 | |
| 0.00 | 1.08 | 0.00 | 1.13 | 20.35 | 62.19 | -62.15 | 70.47 | 0.8815 | -265.0 | -213.7 | |
| 12.07 | -2.00 | 11.83 | -2.00 | 15.64 | 64.06 | -60.27 | 75.79 | 0.8647 | -392.7 | 999999 | |
| 0.00 | 1.26 | 0.00 | 1.30 | 18.19 | 62.24 | -62.09 | 72.92 | 0.8802 | -336.0 | -298.6 | |
| 0.00 | 2.88 | 0.00 | 2.95 | 15.01 | 62.53 | -61.80 | 76.54 | 0.8772 | -550.0 | -379.8 | |
| 1.71 | 56.65 | 1.84 | 60.89 | 17.18 | 61.04 | -63.29 | 74.10 | 0.8893 | -443.7 | 1.3 | |
| 0.00 | 4.77 | 0.00 | 4.95 | 15.10 | 62.15 | -62.18 | 76.44 | 0.8803 | 89.0 | 83.6 | |
| 11.62 | -7.00 | 12.40 | -7.00 | 16.64 | 61.23 | -63.10 | 74.71 | 0.8877 | -636.6 | 999999 | |
| 0.00 | 2.70 | 0.00 | 2.81 | 14.81 | 62.03 | -62.30 | 76.78 | 0.8813 | 343.0 | 281.1 | |
| 0.00 | 0.90 | 0.00 | 0.91 | 12.90 | 62.85 | -61.48 | 78.96 | 0.8746 | -188.0 | -182.6 | |
| 0.00 | 1.17 | 0.00 | 1.23 | 14.93 | 61.76 | -62.57 | 76.63 | 0.8834 | 378.0 | 355.6 | |
| 0.00 | 1.26 | 0.00 | 1.40 | 17.83 | 59.97 | -64.37 | 73.40 | 0.8974 | -407.0 | -285.6 | |
| 0.00 | 4.14 | 0.00 | 4.53 | 14.84 | 60.54 | -63.79 | 76.74 | 0.8929 | 374.0 | 404.8 | |
| 0.00 | 8.56 | 0.00 | 9.49 | 15.35 | 60.04 | -64.29 | 76.17 | 0.8967 | 763.0 | 570.5 | |
| 5.49 | 16.03 | 6.16 | 18.14 | 15.00 | 59.72 | -64.61 | 76.55 | 0.8990 | 785.8 | 512.1 | |
| 0.00 | 1.17 | 0.00 | 1.33 | 15.41 | 59.41 | -64.92 | 76.10 | 0.9013 | 588.0 | 558.6 | |
| 1.44 | -16.00 | 1.64 | -16.00 | 15.22 | 59.37 | -64.96 | 76.31 | 0.9016 | 591.8 | 999999 | |
| 0.00 | 1.17 | 0.00 | 1.35 | 15.63 | 58.82 | -65.51 | 75.86 | 0.9056 | 603.0 | 532.8 | |
| 2.16 | 3.24 | 2.50 | 3.74 | 15.29 | 58.87 | -65.46 | 76.23 | 0.9052 | 525.2 | 559.2 | |
| 0.00 | 1.35 | 0.00 | 1.59 | 16.12 | 58.36 | -65.98 | 75.32 | 0.9088 | 535.0 | 467.0 | |
| 0.00 | 1.17 | 0.00 | 1.38 | 15.81 | 58.40 | -65.93 | 75.66 | 0.9085 | 512.0 | 512.8 | |
| 0.00 | 0.81 | 0.00 | 0.95 | 15.48 | 58.60 | -65.73 | 76.02 | 0.9071 | 517.0 | 386.0 | |
| 0.00 | 1.08 | 0.00 | 1.38 | 18.70 | 56.17 | -68.16 | 72.50 | 0.9235 | 590.0 | 491.1 | |
| 0.00 | 1.35 | 0.00 | 1.74 | 18.90 | 55.92 | -68.42 | 72.29 | 0.9251 | 437.0 | 397.2 | |
| 0.00 | 1.26 | 0.00 | 1.47 | 14.72 | 58.52 | -65.81 | 76.86 | 0.9077 | 418.0 | 355.6 | |
| 0.00 | 1.44 | 0.00 | 1.73 | 15.77 | 57.79 | -66.54 | 75.70 | 0.9128 | 290.0 | 261.6 | |
| 0.00 | 1.80 | 0.00 | 2.33 | 18.00 | 55.89 | -68.45 | 73.26 | 0.9253 | 504.0 | 481.0 | |
| 1.89 | 4.95 | 2.57 | 6.70 | 18.93 | 54.71 | -69.62 | 72.27 | 0.9325 | 143.3 | 204.9 | |
| 0.00 | 1.80 | 0.00 | 2.18 | 15.19 | 57.60 | -66.73 | 76.33 | 0.9141 | 448.0 | 362.1 | |
| 0.00 | 1.62 | 0.00 | 2.11 | 17.76 | 55.73 | -68.60 | 73.52 | 0.9263 | 388.0 | 330.0 | |
| 3.78 | 10.45 | 5.04 | 13.96 | 18.18 | 55.20 | -69.14 | 73.07 | 0.9296 | 468.7 | 205.7 | |
| 0.00 | 0.81 | 0.00 | 0.99 | 14.95 | 57.43 | -66.90 | 76.59 | 0.9153 | 199.0 | 210.9 | |
| 0.00 | 1.08 | 0.00 | 1.46 | 17.90 | 54.90 | -69.44 | 73.37 | 0.9314 | -280.0 | -238.7 | |
| 0.00 | 0.72 | 0.00 | 0.96 | 17.75 | 55.02 | -69.31 | 73.53 | 0.9307 | 70.0 | 158.8 | |
| 14.05 | 108.17 | 17.98 | 139.61 | 13.91 | 56.18 | -68.16 | 77.70 | 0.9238 | 714.3 | 78.3 | |
| 3.87 | -36.00 | 5.03 | -36.00 | 13.93 | 55.82 | -68.51 | 77.66 | 0.9261 | -262.6 | 999999 | |
| 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. | |