| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 100.46 | 302.97 | 110.97 | 330.39 | 5.45 | 11.03 | 61.83 | 279.90 | 0.8924 | 122.3 | 113.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.60 | 9.20 | 6.29 | 12.60 | 4.79 | 17.00 | 67.80 | 278.01 | 0.9333 | -382.2 | -162.0 | |
| 0.00 | 1.22 | 0.00 | 1.51 | 5.10 | 14.77 | 65.57 | 278.76 | 0.9193 | -489.0 | -393.4 | |
| 0.00 | 1.39 | 0.00 | 1.69 | 5.77 | 13.98 | 64.78 | 279.64 | 0.9147 | -326.0 | -227.4 | |
| 8.42 | 17.11 | 10.18 | 20.66 | 6.15 | 13.78 | 64.58 | 280.08 | 0.9138 | -363.4 | -187.2 | |
| 0.00 | 2.43 | 0.00 | 2.74 | 4.42 | 12.21 | 63.01 | 278.51 | 0.9002 | -118.0 | -83.8 | |
| 28.83 | 40.81 | 32.01 | 45.32 | 3.80 | 11.86 | 62.66 | 277.91 | 0.8967 | -451.2 | -276.7 | |
| 2.69 | 230.81 | 2.97 | 245.87 | 5.00 | 11.45 | 62.25 | 279.31 | 0.8953 | 222.6 | 179.2 | |
| 23.79 | -7.00 | 25.72 | -7.00 | 5.95 | 10.67 | 61.47 | 280.51 | 0.8906 | 510.0 | 999999 | |
| 1.56 | -7.00 | 1.66 | -7.00 | 5.06 | 10.38 | 61.18 | 279.60 | 0.8870 | 234.8 | 999999 | |
| 1.13 | -7.00 | 1.19 | -7.00 | 4.34 | 10.21 | 61.01 | 278.84 | 0.8846 | -80.2 | 999999 | |
| 4.69 | -7.00 | 4.92 | -7.00 | 4.56 | 9.99 | 60.79 | 279.13 | 0.8832 | 462.4 | 999999 | |
| 4.69 | -7.00 | 4.89 | -7.00 | 4.94 | 9.80 | 60.60 | 279.58 | 0.8822 | 610.3 | 999999 | |
| 18.58 | -7.00 | 19.61 | -7.00 | 6.28 | 9.86 | 60.66 | 281.07 | 0.8848 | 764.2 | 999999 | |
| 1.48 | -7.00 | 1.53 | -7.00 | 4.82 | 9.60 | 60.40 | 279.50 | 0.8804 | 718.8 | 999999 | |
| 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. | |