| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 70.99 | 375.05 | 38.24 | 202.07 | -16.27 | 12.30 | 20.36 | 238.19 | 0.3945 | 874.8 | 405.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.13 | 219.30 | 17.42 | 118.95 | -16.54 | 13.20 | 21.26 | 238.68 | 0.4087 | 1196.2 | 402.5 | |
| 3.83 | -1.00 | 2.07 | -1.00 | -16.55 | 12.84 | 20.90 | 238.26 | 0.4039 | 1366.6 | 999999 | |
| 2.38 | -1.00 | 1.29 | -1.00 | -16.68 | 12.56 | 20.62 | 237.66 | 0.4010 | 1143.6 | 999999 | |
| 0.60 | 1.62 | 0.32 | 0.86 | -14.90 | 11.72 | 19.78 | 240.81 | 0.3763 | -438.3 | -274.1 | |
| 0.00 | 3.66 | 0.00 | 1.97 | -16.82 | 11.79 | 19.85 | 236.44 | 0.3917 | 724.0 | 569.9 | |
| 32.05 | 140.34 | 17.14 | 75.01 | -15.81 | 11.45 | 19.51 | 238.35 | 0.3792 | 1274.1 | 482.3 | |
| 0.00 | 1.87 | 0.00 | 1.00 | -14.73 | 11.35 | 19.41 | 240.81 | 0.3698 | 858.0 | 695.3 | |
| 0.00 | 1.45 | 0.00 | 0.75 | -16.30 | 6.65 | 14.71 | 229.97 | 0.3197 | -746.0 | -610.8 | |
| 0.00 | 1.19 | 0.00 | 0.62 | -17.00 | 6.60 | 14.67 | 228.20 | 0.3263 | -891.0 | -703.8 | |
| 0.00 | 1.19 | 0.00 | 0.62 | -16.27 | 5.03 | 13.09 | 226.88 | 0.2993 | -880.0 | -732.1 | |
| 0.00 | 1.45 | 0.00 | 0.76 | -19.16 | 4.22 | 12.28 | 218.51 | 0.3241 | -876.0 | -568.5 | |
| 0.00 | 0.85 | 0.00 | 0.44 | -16.62 | 3.79 | 11.86 | 223.25 | 0.2886 | -773.0 | -544.7 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -17.83 | 3.62 | 11.68 | 219.98 | 0.3013 | -771.0 | -639.3 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -15.41 | 2.29 | 10.35 | 222.64 | 0.2569 | -846.0 | -564.1 | |
| 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. | |