| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.22 | 144.48 | 43.36 | 128.19 | 18.88 | 171.78 | 53.86 | 292.72 | 0.8291 | -190.2 | 59.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 4.35 | 0.00 | 4.21 | 18.30 | 175.47 | 57.55 | 291.13 | 0.8611 | -98.0 | -109.4 | |
| 0.00 | 1.79 | 0.00 | 1.69 | 17.12 | 174.71 | 56.80 | 289.93 | 0.8527 | 378.0 | 312.4 | |
| 13.48 | 53.31 | 13.01 | 51.76 | 18.86 | 175.24 | 57.33 | 291.82 | 0.8601 | -673.2 | -44.4 | |
| 2.81 | -3.00 | 2.71 | -3.00 | 19.14 | 175.05 | 57.13 | 292.18 | 0.8590 | -658.9 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.92 | 18.69 | 172.52 | 54.60 | 292.24 | 0.8364 | -329.0 | -291.3 | |
| 0.00 | 0.51 | 0.00 | 0.46 | 19.50 | 172.70 | 54.78 | 293.14 | 0.8397 | -383.0 | -353.0 | |
| 10.07 | 15.78 | 8.99 | 14.13 | 19.00 | 172.18 | 54.27 | 292.69 | 0.8341 | -810.7 | -456.7 | |
| 5.46 | 9.21 | 4.60 | 7.78 | 18.11 | 169.95 | 52.03 | 292.21 | 0.8116 | -641.2 | -335.5 | |
| 0.00 | 1.19 | 0.00 | 1.02 | 19.07 | 170.17 | 52.25 | 293.31 | 0.8159 | -440.0 | -330.1 | |
| 0.00 | 1.02 | 0.00 | 0.86 | 18.45 | 169.84 | 51.93 | 292.65 | 0.8114 | 50.0 | 32.8 | |
| 0.00 | 0.68 | 0.00 | 0.57 | 18.55 | 169.48 | 51.56 | 292.86 | 0.8082 | 269.0 | 188.9 | |
| 0.00 | 0.94 | 0.00 | 0.80 | 19.95 | 170.11 | 52.19 | 294.37 | 0.8175 | -66.0 | -109.0 | |
| 14.59 | 51.95 | 11.80 | 41.86 | 18.93 | 167.80 | 49.89 | 293.81 | 0.7931 | 658.3 | 346.5 | |
| 2.81 | -13.00 | 2.25 | -13.00 | 19.22 | 167.05 | 49.13 | 294.40 | 0.7864 | 733.2 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.75 | 20.60 | 166.76 | 48.85 | 296.19 | 0.7878 | 557.0 | 486.0 | |
| 0.00 | 1.02 | 0.00 | 0.79 | 20.29 | 164.98 | 47.07 | 296.44 | 0.7692 | 560.0 | 508.8 | |
| 0.00 | 0.77 | 0.00 | 0.59 | 20.48 | 164.82 | 46.91 | 296.73 | 0.7683 | 525.0 | 475.4 | |
| 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. | |