| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.45 | 323.30 | 36.89 | 258.37 | 22.97 | 156.26 | -50.93 | 65.80 | 0.7858 | -726.5 | -232.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.06 | 0.00 | 0.85 | 25.41 | 156.16 | -51.03 | 62.78 | 0.7920 | -628.0 | -532.9 | |
| 14.25 | 250.90 | 11.19 | 198.56 | 22.50 | 156.96 | -50.22 | 66.25 | 0.7780 | -1022.8 | -279.2 | |
| 21.64 | -2.00 | 17.17 | -2.00 | 22.97 | 156.52 | -50.67 | 65.75 | 0.7834 | -916.6 | 999999 | |
| 3.52 | -2.00 | 2.77 | -2.00 | 22.06 | 156.67 | -50.52 | 66.87 | 0.7801 | -730.8 | 999999 | |
| 4.57 | 59.82 | 3.75 | 49.23 | 24.09 | 155.11 | -52.08 | 64.64 | 0.7991 | -871.6 | -153.1 | |
| 1.94 | -5.00 | 1.59 | -5.00 | 23.86 | 154.97 | -52.21 | 64.96 | 0.8000 | -741.2 | 999999 | |
| 0.00 | 1.23 | 0.00 | 1.01 | 23.47 | 154.93 | -52.26 | 65.45 | 0.7997 | -461.0 | -369.6 | |
| 0.53 | 3.69 | 0.42 | 2.97 | 20.18 | 155.31 | -51.88 | 69.49 | 0.7907 | 600.7 | 461.0 | |
| 0.00 | 0.97 | 0.00 | 0.79 | 21.10 | 154.75 | -52.44 | 68.42 | 0.7975 | -620.0 | -434.5 | |
| 0.00 | 1.32 | 0.00 | 1.13 | 23.81 | 152.97 | -54.22 | 65.40 | 0.8185 | 494.0 | 452.3 | |
| 0.00 | 1.58 | 0.00 | 1.37 | 23.70 | 152.52 | -54.67 | 65.61 | 0.8224 | 633.0 | 525.2 | |
| 0.00 | 1.67 | 0.00 | 1.45 | 23.24 | 152.40 | -54.78 | 66.18 | 0.8227 | 443.0 | 384.0 | |
| 0.00 | 1.06 | 0.00 | 1.01 | 26.91 | 148.88 | -58.30 | 62.44 | 0.8579 | 327.0 | 284.5 | |
| 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. | |