| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42 | 221 | 22 | 117 | 11.48 | 212.15 | 18.16 | 295.37 | 0.3398 | 128.5 | 276.4 | |
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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 | 9.42 | 214.17 | 20.18 | 287.63 | 0.3587 | 649.0 | 498.3 | |
| 8 | 91 | 4 | 49 | 10.54 | 214.16 | 20.17 | 290.62 | 0.3638 | 1119.1 | 993.0 | |
| 15 | -2 | 8 | -2 | 10.78 | 213.72 | 19.73 | 291.65 | 0.3584 | 1385.5 | 999999 | |
| 0 | 5 | 0 | 2 | 9.51 | 213.35 | 19.36 | 288.51 | 0.3463 | 710.0 | 675.8 | |
| 0 | 5 | 0 | 3 | 11.30 | 213.13 | 19.14 | 293.58 | 0.3524 | 691.0 | 578.7 | |
| 0 | 10 | 0 | 5 | 10.69 | 212.64 | 18.65 | 292.41 | 0.3414 | 1105.0 | 817.8 | |
| 0 | 10 | 0 | 5 | 12.71 | 212.53 | 18.54 | 297.94 | 0.3526 | 947.0 | 636.2 | |
| 0 | 7 | 0 | 4 | 11.78 | 212.46 | 18.47 | 295.56 | 0.3453 | 524.0 | 326.9 | |
| 0 | 3 | 0 | 2 | 10.66 | 212.26 | 18.27 | 292.70 | 0.3355 | 584.0 | 515.2 | |
| 0 | 3 | 0 | 2 | 12.42 | 211.14 | 17.15 | 298.92 | 0.3305 | -452.0 | -508.8 | |
| 13 | 45 | 7 | 24 | 13.03 | 210.15 | 16.16 | 301.95 | 0.3211 | -1458.4 | -510.9 | |
| 0 | 5 | 0 | 2 | 11.51 | 209.81 | 15.82 | 298.15 | 0.3044 | -763.0 | -368.0 | |
| 4 | -11 | 2 | -11 | 13.26 | 209.88 | 15.89 | 303.01 | 0.3193 | -703.8 | 999999 | |
| 2 | 14 | 1 | 7 | 12.25 | 209.78 | 15.79 | 300.36 | 0.3095 | -1225.2 | -988.7 | |
| 0 | 10 | 0 | 5 | 10.90 | 209.66 | 15.67 | 296.51 | 0.2977 | -1149.0 | -985.6 | |
| 0 | 9 | 0 | 5 | 11.87 | 209.26 | 15.27 | 300.03 | 0.2991 | -894.0 | -829.6 | |
| 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. | |