| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.41 | 33.54 | 4.99 | 17.75 | -14.74 | 3.67 | 3.17 | 188.54 | 0.3539 | -4.5 | -249.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.48 | 0.00 | 0.80 | -16.65 | 6.71 | 6.21 | 195.36 | 0.3928 | 805.0 | 568.2 | |
| 2.09 | 3.05 | 1.11 | 1.62 | -14.88 | 6.28 | 5.78 | 195.61 | 0.3634 | 920.4 | 726.3 | |
| 5.92 | 6.88 | 3.14 | 3.65 | -14.63 | 6.12 | 5.62 | 195.39 | 0.3586 | 1041.2 | 935.2 | |
| 0.35 | 2.96 | 0.19 | 1.59 | -16.29 | 6.04 | 5.54 | 194.01 | 0.3844 | 836.5 | 739.1 | |
| 0.00 | 1.22 | 0.00 | 0.65 | -15.22 | 3.96 | 3.46 | 189.35 | 0.3605 | 745.0 | 613.4 | |
| 0.00 | 0.96 | 0.00 | 0.51 | -16.79 | 3.36 | 2.87 | 187.19 | 0.3844 | 824.0 | 609.3 | |
| 0.00 | 1.31 | 0.00 | 0.69 | -15.02 | 2.35 | 1.85 | 185.08 | 0.3540 | -815.0 | -641.7 | |
| 0.00 | 1.13 | 0.00 | 0.60 | -15.14 | 2.32 | 1.82 | 184.96 | 0.3560 | -655.0 | -557.8 | |
| 0.00 | 1.22 | 0.00 | 0.64 | -13.62 | 1.88 | 1.38 | 184.08 | 0.3304 | -1041.0 | -864.1 | |
| 0.00 | 1.22 | 0.00 | 0.64 | -13.78 | 1.88 | 1.38 | 184.04 | 0.3330 | -851.0 | -705.5 | |
| 0.00 | 2.27 | 0.00 | 1.19 | -14.28 | 1.88 | 1.38 | 183.95 | 0.3413 | -1047.0 | -756.1 | |
| 0.00 | 0.78 | 0.00 | 0.41 | -13.24 | 1.81 | 1.32 | 183.97 | 0.3241 | -957.0 | -722.1 | |
| 0.00 | 2.88 | 0.00 | 1.51 | -13.93 | 1.66 | 1.17 | 183.39 | 0.3354 | -1004.0 | -776.7 | |
| 1.05 | 4.79 | 0.55 | 2.51 | -13.62 | 1.02 | 0.52 | 181.54 | 0.3297 | -995.7 | -796.0 | |
| 0.00 | 1.39 | 0.00 | 0.74 | -16.04 | 359.94 | -0.56 | 178.53 | 0.3694 | -820.0 | -690.3 | |
| 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. | |