| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.01 | 219.27 | 25.26 | 117.53 | -11.69 | 178.63 | -13.17 | 144.34 | 0.3833 | 438.0 | 306.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.76 | 188.77 | 0.94 | 100.81 | -11.94 | 179.46 | -12.34 | 146.33 | 0.3787 | 866.9 | 399.4 | |
| 35.50 | -1.00 | 18.96 | -1.00 | -11.51 | 179.20 | -12.60 | 145.11 | 0.3753 | 1191.0 | 999999 | |
| 0.00 | 4.92 | 0.00 | 2.65 | -12.10 | 178.45 | -13.35 | 144.45 | 0.3900 | 768.0 | 531.1 | |
| 4.22 | 7.56 | 2.30 | 4.11 | -12.78 | 176.60 | -15.20 | 141.94 | 0.4164 | -871.6 | -659.7 | |
| 0.00 | 1.32 | 0.00 | 0.72 | -13.01 | 176.46 | -15.34 | 142.02 | 0.4206 | -735.0 | -617.7 | |
| 0.00 | 1.58 | 0.00 | 0.88 | -14.17 | 174.22 | -17.58 | 139.92 | 0.4566 | -837.0 | -596.3 | |
| 0.00 | 0.44 | 0.00 | 0.25 | -14.37 | 173.91 | -17.89 | 139.72 | 0.4621 | -527.0 | -460.0 | |
| 1.49 | 3.52 | 0.82 | 1.94 | -12.12 | 173.63 | -18.17 | 135.84 | 0.4394 | -964.5 | -853.4 | |
| 2.72 | 3.60 | 1.51 | 1.99 | -12.57 | 173.57 | -18.23 | 136.45 | 0.4451 | -892.4 | -787.4 | |
| 0.00 | 1.32 | 0.00 | 0.73 | -13.47 | 173.37 | -18.43 | 137.53 | 0.4573 | -724.0 | -594.0 | |
| 1.32 | 1.32 | 0.73 | 0.73 | -13.09 | 173.34 | -18.47 | 136.89 | 0.4533 | -725.9 | 0.0 | |
| 0.00 | 2.55 | 0.00 | 1.41 | -12.64 | 173.30 | -18.50 | 136.15 | 0.4487 | -739.0 | -499.5 | |
| 0.00 | 1.14 | 0.00 | 0.63 | -12.85 | 172.96 | -18.84 | 135.95 | 0.4546 | -652.0 | -562.7 | |
| 0.00 | 1.23 | 0.00 | 0.68 | -11.86 | 172.23 | -19.57 | 133.27 | 0.4522 | -710.0 | -553.9 | |
| 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. | |