| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.86 | 411.35 | 37.92 | 223.39 | 17.72 | 166.61 | 8.13 | 340.79 | 0.4106 | -796.4 | -301.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.86 | 377.79 | 3.19 | 205.34 | 17.87 | 167.51 | 9.03 | 338.92 | 0.4169 | -1120.5 | -394.1 | |
| 58.85 | -1.00 | 31.97 | -1.00 | 17.70 | 167.02 | 8.54 | 339.82 | 0.4117 | -1423.6 | 999999 | |
| 0.00 | 0.80 | 0.00 | 0.43 | 17.67 | 163.55 | 5.06 | 347.67 | 0.3956 | 793.0 | 680.8 | |
| 0.00 | 2.49 | 0.00 | 1.34 | 17.93 | 163.27 | 4.79 | 348.47 | 0.3988 | 940.0 | 772.4 | |
| 0.00 | 0.44 | 0.00 | 0.24 | 18.32 | 163.16 | 4.67 | 348.94 | 0.4046 | 372.0 | 444.2 | |
| 0.00 | 0.98 | 0.00 | 0.53 | 18.62 | 163.13 | 4.65 | 349.14 | 0.4091 | 750.0 | 669.9 | |
| 0.00 | 1.24 | 0.00 | 0.67 | 17.93 | 162.83 | 4.34 | 349.51 | 0.3974 | 962.0 | 812.9 | |
| 0.00 | 2.66 | 0.00 | 1.45 | 19.34 | 162.64 | 4.15 | 350.57 | 0.4191 | 544.0 | 478.4 | |
| 0.00 | 1.07 | 0.00 | 0.57 | 17.93 | 162.48 | 3.99 | 350.34 | 0.3963 | 829.0 | 687.1 | |
| 0.00 | 1.69 | 0.00 | 0.91 | 18.29 | 162.42 | 3.94 | 350.63 | 0.4019 | 839.0 | 715.8 | |
| 0.00 | 1.33 | 0.00 | 0.72 | 17.89 | 162.16 | 3.67 | 351.08 | 0.3950 | 983.0 | 836.2 | |
| 0.00 | 7.19 | 0.00 | 3.86 | 17.37 | 161.30 | 2.81 | 352.99 | 0.3846 | 1015.0 | 797.3 | |
| 1.24 | 4.17 | 0.67 | 2.24 | 17.85 | 160.42 | 1.93 | 355.28 | 0.3910 | 879.0 | 622.9 | |
| 3.91 | 9.50 | 2.09 | 5.09 | 17.36 | 160.25 | 1.77 | 355.58 | 0.3829 | 1103.2 | 779.9 | |
| 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. | |