| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.29 | 0.00 | 12.03 | -9.96 | 331.08 | 15.05 | 220.48 | 0.3954 | 350.6 | 284.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.58 | -11.14 | 342.36 | 26.32 | 235.48 | 0.5301 | 566.0 | 482.6 | |
| 0.00 | 1.62 | 0.00 | 0.89 | -8.87 | 336.94 | 20.90 | 232.99 | 0.4433 | 795.0 | 570.9 | |
| 0.00 | 1.53 | 0.00 | 0.84 | -8.69 | 335.91 | 19.88 | 231.90 | 0.4290 | 885.0 | 754.5 | |
| 0.00 | 2.42 | 0.00 | 1.33 | -8.94 | 335.79 | 19.76 | 231.27 | 0.4299 | 817.0 | 715.2 | |
| 0.00 | 1.62 | 0.00 | 0.88 | -8.53 | 335.77 | 19.74 | 232.00 | 0.4256 | 984.0 | 827.9 | |
| 0.00 | 0.81 | 0.00 | 0.43 | -5.91 | 333.66 | 17.63 | 234.10 | 0.3735 | 806.0 | 648.8 | |
| 0.00 | 0.99 | 0.00 | 0.52 | -7.02 | 330.65 | 14.62 | 226.39 | 0.3474 | 777.0 | 586.3 | |
| 0.00 | 3.95 | 0.00 | 2.10 | -8.80 | 330.49 | 14.46 | 222.55 | 0.3664 | 845.0 | 542.5 | |
| 0.00 | 0.81 | 0.00 | 0.43 | -10.87 | 329.88 | 13.85 | 217.74 | 0.3856 | 665.0 | 513.1 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -10.64 | 329.81 | 13.77 | 217.96 | 0.3821 | 836.0 | 707.3 | |
| 0.00 | 1.44 | 0.00 | 0.80 | -16.78 | 328.22 | 12.19 | 206.76 | 0.4509 | -667.0 | -565.2 | |
| 0.00 | 2.96 | 0.00 | 1.55 | -10.11 | 323.58 | 7.55 | 203.78 | 0.3221 | -804.0 | -603.2 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -11.40 | 322.64 | 6.61 | 199.71 | 0.3362 | -798.0 | -606.9 | |
| 0.00 | 0.99 | 0.00 | 0.53 | -14.56 | 320.05 | 4.02 | 190.47 | 0.3752 | -799.0 | -596.1 | |
| 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. | |