| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 81 | 480 | 50 | 292 | -29.16 | 23.63 | -27.57 | 135.73 | 0.5789 | -937.4 | -318.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9 | 364 | 6 | 217 | -28.63 | 25.95 | -25.25 | 137.05 | 0.5517 | -1659.2 | -548.8 | |
| 45 | -1 | 27 | -1 | -28.69 | 25.31 | -25.89 | 136.49 | 0.5586 | -1658.2 | 999999 | |
| 0 | 7 | 0 | 4 | -28.10 | 22.03 | -29.17 | 132.67 | 0.5869 | 284.0 | 254.2 | |
| 0 | 6 | 0 | 4 | -27.58 | 20.69 | -30.51 | 130.84 | 0.5971 | 347.0 | 281.3 | |
| 8 | 37 | 5 | 24 | -31.02 | 19.31 | -31.89 | 134.47 | 0.6368 | 854.9 | 5.6 | |
| 8 | -5 | 5 | -5 | -31.35 | 19.08 | -32.12 | 134.73 | 0.6415 | -660.5 | 999999 | |
| 0 | 10 | 0 | 6 | -30.23 | 18.87 | -32.33 | 133.10 | 0.6352 | -448.0 | 13.1 | |
| 0 | 3 | 0 | 2 | -31.56 | 17.98 | -33.22 | 134.20 | 0.6535 | 519.0 | 410.2 | |
| 0 | 9 | 0 | 6 | -29.54 | 18.70 | -32.50 | 132.06 | 0.6319 | 696.0 | 651.8 | |
| 0 | 7 | 0 | 4 | -29.38 | 17.97 | -33.23 | 131.32 | 0.6381 | 982.0 | 876.0 | |
| 2 | 29 | 2 | 19 | -31.81 | 16.85 | -34.35 | 133.72 | 0.6659 | 663.3 | 599.1 | |
| 2 | 5 | 1 | 4 | -29.57 | 17.58 | -33.62 | 131.31 | 0.6433 | 782.0 | 783.0 | |
| 0 | 3 | 0 | 2 | -29.94 | 17.33 | -33.87 | 131.63 | 0.6483 | 654.0 | 561.7 | |
| 7 | -11 | 4 | -11 | -31.70 | 16.35 | -34.85 | 133.24 | 0.6698 | 714.5 | 999999 | |
| 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. | |