| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.73 | 32.30 | 4.78 | 17.58 | 10.07 | 179.96 | 21.16 | 300.65 | 0.4157 | -52.9 | -77.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.80 | 0.00 | 0.99 | 7.40 | 183.10 | 24.30 | 291.73 | 0.4412 | -774.0 | -653.5 | |
| 0.00 | 1.80 | 0.00 | 1.00 | 11.63 | 181.80 | 23.01 | 301.57 | 0.4512 | -793.0 | -595.3 | |
| 3.60 | 13.22 | 1.97 | 7.24 | 9.14 | 181.41 | 22.61 | 296.94 | 0.4276 | -1011.9 | -763.6 | |
| 5.13 | -3.00 | 2.81 | -3.00 | 9.42 | 181.36 | 22.56 | 297.57 | 0.4288 | -1056.6 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 9.23 | 181.11 | 22.32 | 297.42 | 0.4240 | -303.0 | -327.5 | |
| 0.00 | 3.06 | 0.00 | 1.67 | 9.50 | 181.07 | 22.27 | 298.06 | 0.4253 | -1031.0 | -835.9 | |
| 0.00 | 0.81 | 0.00 | 0.43 | 6.82 | 178.19 | 19.40 | 295.00 | 0.3654 | 790.0 | 635.8 | |
| 0.00 | 1.44 | 0.00 | 0.78 | 11.43 | 178.40 | 19.60 | 305.28 | 0.4045 | 644.0 | 452.7 | |
| 0.00 | 1.08 | 0.00 | 0.58 | 10.34 | 178.32 | 19.52 | 303.07 | 0.3940 | 684.0 | 572.9 | |
| 0.00 | 1.17 | 0.00 | 0.64 | 14.57 | 178.26 | 19.47 | 311.52 | 0.4326 | 588.0 | 490.6 | |
| 0.00 | 1.35 | 0.00 | 0.73 | 11.14 | 177.59 | 18.79 | 305.79 | 0.3913 | 811.0 | 540.7 | |
| 0.00 | 1.17 | 0.00 | 0.64 | 16.02 | 177.70 | 18.91 | 314.86 | 0.4412 | 783.0 | 553.3 | |
| 0.00 | 1.53 | 0.00 | 0.81 | 9.91 | 176.08 | 17.29 | 305.30 | 0.3602 | 887.0 | 699.5 | |
| 0.00 | 1.62 | 0.00 | 0.86 | 9.85 | 175.89 | 17.09 | 305.45 | 0.3570 | 882.0 | 699.8 | |
| 0.00 | 1.26 | 0.00 | 0.67 | 11.60 | 174.09 | 15.30 | 312.45 | 0.3517 | 853.0 | 769.6 | |
| 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. | |