| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.89 | 30.86 | 2.09 | 17.05 | -17.39 | 98.41 | -14.34 | 148.17 | 0.4393 | -180.9 | 81.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.37 | 12.88 | 1.81 | 6.91 | -16.22 | 103.23 | -9.52 | 155.49 | 0.3846 | 977.1 | 854.7 | |
| 0.00 | 1.21 | 0.00 | 0.66 | -16.39 | 100.47 | -12.28 | 149.80 | 0.4073 | 944.0 | 836.0 | |
| 0.00 | 0.69 | 0.00 | 0.38 | -16.61 | 100.14 | -12.61 | 149.43 | 0.4131 | 929.0 | 851.8 | |
| 0.00 | 1.30 | 0.00 | 0.70 | -16.49 | 99.99 | -12.76 | 148.97 | 0.4126 | 879.0 | 716.1 | |
| 0.52 | 1.47 | 0.28 | 0.80 | -16.49 | 99.77 | -12.98 | 148.54 | 0.4145 | 841.2 | 664.8 | |
| 0.00 | 1.90 | 0.00 | 1.04 | -16.33 | 98.31 | -14.44 | 145.56 | 0.4249 | -856.0 | -762.7 | |
| 0.00 | 1.12 | 0.00 | 0.62 | -16.67 | 95.48 | -17.28 | 141.18 | 0.4557 | -758.0 | -608.2 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -16.98 | 94.40 | -18.35 | 139.95 | 0.4699 | -771.0 | -608.3 | |
| 0.00 | 1.30 | 0.00 | 0.73 | -17.94 | 94.23 | -18.52 | 141.05 | 0.4826 | -902.0 | -737.7 | |
| 0.00 | 1.30 | 0.00 | 0.73 | -18.20 | 94.07 | -18.68 | 141.17 | 0.4872 | -702.0 | -591.7 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -17.66 | 94.13 | -18.62 | 140.50 | 0.4803 | -775.0 | -611.3 | |
| 0.00 | 1.21 | 0.00 | 0.69 | -18.75 | 93.94 | -18.81 | 141.71 | 0.4948 | -790.0 | -639.3 | |
| 0.00 | 0.61 | 0.00 | 0.34 | -17.61 | 93.54 | -19.21 | 139.57 | 0.4855 | -684.0 | -594.0 | |
| 0.00 | 1.47 | 0.00 | 0.86 | -19.91 | 90.66 | -22.09 | 138.80 | 0.5390 | -734.0 | -597.9 | |
| 0.00 | 1.21 | 0.00 | 0.71 | -19.59 | 90.60 | -22.15 | 138.30 | 0.5361 | -719.0 | -659.3 | |
| 0.00 | 0.69 | 0.00 | 0.43 | -23.77 | 88.84 | -23.91 | 141.34 | 0.5960 | -712.0 | -562.6 | |
| 0.00 | 0.52 | 0.00 | 0.34 | -27.54 | 87.49 | -25.26 | 143.98 | 0.6457 | -467.0 | -457.8 | |
| 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. | |