| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.53 | 0.00 | 10.40 | 11.00 | 96.99 | 9.02 | 233.04 | 0.2082 | -357.4 | -314.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.16 | 0.00 | 1.63 | 8.89 | 103.48 | 15.50 | 280.46 | 0.2698 | -976.0 | -810.4 | |
| 0.00 | 1.23 | 0.00 | 0.63 | 8.72 | 103.25 | 15.28 | 279.94 | 0.2656 | -967.0 | -818.1 | |
| 0.00 | 2.02 | 0.00 | 1.03 | 9.34 | 102.52 | 14.55 | 282.75 | 0.2553 | 894.0 | 686.0 | |
| 0.00 | 0.79 | 0.00 | 0.40 | 10.07 | 100.09 | 12.11 | 288.13 | 0.2184 | -935.0 | -786.7 | |
| 0.00 | 1.14 | 0.00 | 0.58 | 10.33 | 98.89 | 10.91 | 291.10 | 0.2005 | -812.0 | -674.5 | |
| 0.00 | 1.05 | 0.00 | 0.53 | 10.16 | 98.72 | 10.75 | 290.52 | 0.1969 | -988.0 | -841.1 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 10.40 | 98.70 | 10.73 | 291.71 | 0.1980 | -1007.0 | -865.5 | |
| 0.00 | 2.19 | 0.00 | 1.11 | 10.07 | 98.60 | 10.62 | 290.30 | 0.1944 | -1050.0 | -892.2 | |
| 0.00 | 1.05 | 0.00 | 0.53 | 10.68 | 98.19 | 10.21 | 294.02 | 0.1916 | -806.0 | -706.7 | |
| 0.00 | 1.32 | 0.00 | 0.66 | 9.47 | 97.25 | 9.28 | 289.47 | 0.1694 | -937.0 | -804.7 | |
| 0.00 | 0.79 | 0.00 | 0.40 | 11.89 | 96.46 | 8.49 | 304.17 | 0.1754 | -899.0 | -770.6 | |
| 0.00 | 0.61 | 0.00 | 0.31 | 17.66 | 93.15 | 5.18 | 336.40 | 0.2159 | 689.0 | 584.3 | |
| 0.00 | 0.79 | 0.00 | 0.39 | 13.77 | 87.37 | -0.60 | 4.52 | 0.1306 | 863.0 | 704.9 | |
| 0.00 | 0.61 | 0.00 | 0.31 | 15.10 | 87.12 | -0.85 | 5.39 | 0.1540 | 746.0 | 691.1 | |
| 0.00 | 2.90 | 0.00 | 1.45 | 14.82 | 84.17 | -3.80 | 23.41 | 0.1620 | 824.0 | 632.4 | |
| 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. | |