| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.61 | 232.25 | 55.34 | 274.09 | 3.25 | 162.78 | 65.20 | 273.20 | 0.9089 | -347.2 | -155.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.92 | 201.98 | 20.80 | 244.42 | 2.53 | 163.86 | 66.27 | 272.38 | 0.9171 | -532.7 | -190.9 | |
| 21.54 | -1.00 | 25.77 | -1.00 | 3.37 | 163.15 | 65.57 | 273.31 | 0.9121 | -548.5 | 999999 | |
| 0.00 | 1.45 | 0.00 | 1.70 | 4.33 | 162.51 | 64.92 | 274.37 | 0.9076 | -325.0 | -278.7 | |
| 0.00 | 0.26 | 0.00 | 0.30 | 4.04 | 162.32 | 64.73 | 274.05 | 0.9062 | -423.0 | -411.7 | |
| 0.00 | 2.31 | 0.00 | 2.47 | 3.89 | 159.94 | 62.36 | 273.93 | 0.8879 | -562.0 | -511.6 | |
| 0.00 | 1.11 | 0.00 | 1.19 | 3.71 | 159.92 | 62.34 | 273.73 | 0.8876 | -449.0 | -450.7 | |
| 0.77 | 1.54 | 0.82 | 1.63 | 4.43 | 159.76 | 62.18 | 274.54 | 0.8865 | 144.6 | 88.0 | |
| 0.94 | 2.14 | 0.99 | 2.24 | 4.52 | 159.39 | 61.81 | 274.66 | 0.8835 | 378.1 | 356.1 | |
| 0.00 | 0.26 | 0.00 | 0.26 | 4.44 | 158.63 | 61.05 | 274.59 | 0.8772 | 249.0 | 204.7 | |
| 0.00 | 1.03 | 0.00 | 1.01 | 3.51 | 157.54 | 59.96 | 273.55 | 0.8677 | 451.0 | 385.0 | |
| 1.03 | 2.39 | 0.98 | 2.28 | 5.79 | 156.10 | 58.52 | 276.25 | 0.8556 | 536.2 | 396.1 | |
| 5.04 | 15.98 | 4.71 | 14.94 | 6.33 | 155.46 | 57.88 | 276.92 | 0.8500 | 723.1 | 426.9 | |
| 0.77 | -12.00 | 0.72 | -12.00 | 6.69 | 155.41 | 57.83 | 277.34 | 0.8498 | 424.4 | 999999 | |
| 0.60 | 1.80 | 0.55 | 1.65 | 4.08 | 155.02 | 57.43 | 274.28 | 0.8451 | 454.3 | 462.4 | |
| 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. | |