| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.54 | 273.67 | 26.80 | 148.04 | -24.09 | 191.53 | 9.60 | 202.31 | 0.4031 | 772.0 | 337.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.98 | 260.62 | 9.73 | 141.04 | -24.02 | 192.02 | 10.09 | 203.40 | 0.4048 | 1202.2 | 393.6 | |
| 29.22 | -1.00 | 15.81 | -1.00 | -24.12 | 191.63 | 9.70 | 202.48 | 0.4038 | 1266.4 | 999999 | |
| 1.26 | -1.00 | 0.68 | -1.00 | -23.86 | 191.07 | 9.14 | 201.58 | 0.3967 | 929.6 | 999999 | |
| 1.08 | -1.00 | 0.58 | -1.00 | -23.83 | 190.73 | 8.80 | 200.89 | 0.3942 | 875.7 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.43 | -22.15 | 190.62 | 8.69 | 202.43 | 0.3686 | -660.0 | -495.7 | |
| 0.00 | 0.99 | 0.00 | 0.53 | -22.28 | 190.43 | 8.50 | 201.84 | 0.3693 | -768.0 | -638.6 | |
| 0.00 | 0.81 | 0.00 | 0.43 | -22.47 | 190.41 | 8.48 | 201.58 | 0.3721 | -510.0 | -406.0 | |
| 0.00 | 0.72 | 0.00 | 0.39 | -26.13 | 190.38 | 8.45 | 198.10 | 0.4266 | 631.0 | 482.8 | |
| 0.00 | 2.16 | 0.00 | 1.15 | -23.88 | 187.49 | 5.56 | 193.57 | 0.3794 | -847.0 | -730.3 | |
| 0.00 | 3.60 | 0.00 | 1.92 | -24.01 | 186.56 | 4.64 | 191.30 | 0.3782 | -828.0 | -714.4 | |
| 0.00 | 1.89 | 0.00 | 1.02 | -25.78 | 185.95 | 4.02 | 189.03 | 0.4046 | -774.0 | -594.3 | |
| 0.00 | 1.26 | 0.00 | 0.68 | -25.75 | 185.65 | 3.72 | 188.37 | 0.4033 | -916.0 | -710.6 | |
| 0.00 | 0.81 | 0.00 | 0.45 | -28.22 | 185.04 | 3.11 | 186.25 | 0.4410 | -548.0 | -375.6 | |
| 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. | |