| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.72 | 0.00 | 12.24 | 7.82 | 136.13 | 3.02 | 348.73 | 0.2814 | 14.6 | 90.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.12 | 0.00 | 0.58 | 8.12 | 143.21 | 10.10 | 326.53 | 0.3163 | -785.0 | -610.3 | |
| 0.00 | 2.07 | 0.00 | 1.06 | 5.02 | 142.69 | 9.58 | 321.75 | 0.2690 | -650.0 | -597.0 | |
| 0.00 | 1.47 | 0.00 | 0.76 | 6.48 | 142.57 | 9.46 | 325.23 | 0.2876 | -953.0 | -695.2 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 6.63 | 142.54 | 9.43 | 325.61 | 0.2894 | -561.0 | -506.7 | |
| 0.00 | 3.10 | 0.00 | 1.60 | 6.88 | 140.88 | 7.77 | 331.03 | 0.2784 | -1061.0 | -796.9 | |
| 0.00 | 0.52 | 0.00 | 0.27 | 6.29 | 140.63 | 7.52 | 330.79 | 0.2678 | -588.0 | -644.5 | |
| 0.00 | 1.21 | 0.00 | 0.63 | 8.80 | 139.95 | 6.84 | 336.84 | 0.3006 | -767.0 | -649.5 | |
| 0.00 | 0.43 | 0.00 | 0.22 | 10.75 | 135.72 | 2.61 | 351.75 | 0.3130 | 508.0 | 353.4 | |
| 0.00 | 1.38 | 0.00 | 0.71 | 7.86 | 134.64 | 1.53 | 354.19 | 0.2628 | 929.0 | 633.7 | |
| 0.00 | 1.47 | 0.00 | 0.75 | 7.49 | 132.90 | -0.21 | 0.80 | 0.2552 | 600.0 | 541.1 | |
| 0.00 | 1.98 | 0.00 | 1.03 | 9.84 | 132.30 | -0.81 | 2.71 | 0.2951 | 730.0 | 639.7 | |
| 0.00 | 1.38 | 0.00 | 0.71 | 8.36 | 131.88 | -1.23 | 4.50 | 0.2706 | 924.0 | 705.2 | |
| 0.00 | 3.79 | 0.00 | 1.96 | 8.52 | 129.93 | -3.18 | 11.43 | 0.2779 | 990.0 | 852.5 | |
| 0.00 | 2.59 | 0.00 | 1.34 | 8.99 | 129.78 | -3.33 | 11.63 | 0.2861 | 889.0 | 772.2 | |
| 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. | |