| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.34 | 51.79 | 13.65 | 33.25 | 8.60 | 3.70 | 39.30 | 279.93 | 0.6380 | -39.1 | -104.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.57 | 8.31 | 6.31 | 41.91 | 279.09 | 0.6717 | -688.0 | -522.9 | |
| 0.00 | 2.93 | 0.00 | 1.93 | 8.39 | 5.60 | 41.20 | 279.30 | 0.6627 | -602.0 | -484.0 | |
| 0.00 | 1.89 | 0.00 | 1.24 | 8.01 | 5.31 | 40.91 | 278.77 | 0.6585 | -613.0 | -499.6 | |
| 3.53 | 19.87 | 2.30 | 12.93 | 8.06 | 4.92 | 40.52 | 278.88 | 0.6535 | -846.3 | -591.9 | |
| 5.76 | -4.00 | 3.75 | -4.00 | 8.07 | 4.65 | 40.25 | 278.93 | 0.6499 | -919.6 | 999999 | |
| 1.81 | -4.00 | 1.17 | -4.00 | 8.16 | 4.50 | 40.10 | 279.10 | 0.6481 | -835.5 | 999999 | |
| 0.86 | 4.04 | 0.56 | 2.61 | 8.14 | 4.15 | 39.75 | 279.12 | 0.6434 | -829.8 | -576.1 | |
| 0.00 | 0.77 | 0.00 | 0.50 | 8.38 | 4.18 | 39.78 | 279.48 | 0.6440 | -737.0 | -590.4 | |
| 0.00 | 1.12 | 0.00 | 0.72 | 9.60 | 3.52 | 39.12 | 281.49 | 0.6371 | 666.0 | 504.7 | |
| 0.00 | 1.29 | 0.00 | 0.82 | 9.52 | 3.08 | 38.68 | 281.46 | 0.6312 | 481.0 | 402.9 | |
| 0.86 | 2.15 | 0.54 | 1.35 | 9.40 | 2.22 | 37.82 | 281.43 | 0.6195 | 870.1 | 750.0 | |
| 0.00 | 2.58 | 0.00 | 1.63 | 9.91 | 2.21 | 37.81 | 282.25 | 0.6203 | 886.0 | 735.0 | |
| 0.00 | 0.95 | 0.00 | 0.60 | 9.67 | 2.18 | 37.78 | 281.88 | 0.6194 | 745.0 | 610.7 | |
| 0.00 | 1.55 | 0.00 | 0.98 | 10.15 | 2.17 | 37.77 | 282.65 | 0.6202 | 668.0 | 581.9 | |
| 8.52 | 11.79 | 5.33 | 7.37 | 8.94 | 1.78 | 37.38 | 280.77 | 0.6128 | 877.1 | 602.4 | |
| 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. | |