| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74 | 453 | 53 | 319 | 18.99 | 31.33 | -43.77 | 66.40 | 0.7154 | 348.4 | -9.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 2 | 18.07 | 41.10 | -34.01 | 63.65 | 0.5956 | 689.0 | 618.8 | |
| 0 | 4 | 0 | 2 | 18.24 | 38.60 | -36.50 | 64.66 | 0.6274 | 648.0 | 469.1 | |
| 29 | 138 | 20 | 93 | 19.54 | 34.60 | -40.51 | 64.51 | 0.6804 | 1176.2 | 485.7 | |
| -3 | -3 | -3 | -3 | 19.74 | 34.26 | -40.84 | 64.37 | 0.6850 | 999999 | 999999 | |
| 0 | 3 | 0 | 2 | 20.70 | 33.33 | -41.78 | 63.41 | 0.6992 | 521.0 | 456.5 | |
| 0 | 2 | 0 | 1 | 20.37 | 33.33 | -41.78 | 63.87 | 0.6980 | 486.0 | 460.4 | |
| 10 | 34 | 7 | 24 | 20.54 | 32.35 | -42.76 | 64.02 | 0.7095 | 808.3 | 213.5 | |
| 0 | 5 | 0 | 3 | 18.16 | 32.89 | -42.21 | 67.10 | 0.6954 | -759.0 | -647.0 | |
| 2 | 11 | 2 | 8 | 19.45 | 32.03 | -43.08 | 65.62 | 0.7094 | 418.3 | 232.2 | |
| 3 | 24 | 2 | 17 | 18.01 | 31.16 | -43.94 | 67.87 | 0.7147 | -854.1 | -681.5 | |
| 0 | 3 | 0 | 2 | 19.60 | 30.63 | -44.47 | 65.89 | 0.7254 | 106.0 | 34.6 | |
| 15 | 204 | 11 | 149 | 18.24 | 29.79 | -45.31 | 67.97 | 0.7307 | -1160.8 | -274.4 | |
| 6 | -12 | 4 | -12 | 18.77 | 29.55 | -45.55 | 67.34 | 0.7348 | -719.9 | 999999 | |
| 0 | 7 | 0 | 5 | 19.25 | 29.26 | -45.84 | 66.78 | 0.7393 | 296.0 | 163.9 | |
| 9 | -12 | 7 | -12 | 18.84 | 28.31 | -46.79 | 67.60 | 0.7484 | 896.0 | 999999 | |
| 0 | 5 | 0 | 4 | 17.58 | 27.84 | -47.27 | 69.37 | 0.7504 | -772.0 | -616.6 | |
| 0 | 9 | 0 | 7 | 17.36 | 27.42 | -47.68 | 69.77 | 0.7544 | -432.0 | -389.4 | |
| 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. | |