| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.01 | 361.45 | 42.29 | 227.75 | 14.86 | 133.27 | 37.92 | 285.60 | 0.6188 | -551.2 | -297.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.26 | 0.00 | 0.84 | 17.62 | 136.46 | 41.11 | 289.20 | 0.6659 | 502.0 | 458.9 | |
| 0.00 | 1.44 | 0.00 | 0.92 | 14.13 | 134.58 | 39.23 | 284.28 | 0.6351 | -268.0 | -297.8 | |
| 52.23 | 320.16 | 33.26 | 203.82 | 15.34 | 134.07 | 38.72 | 286.29 | 0.6307 | -1270.2 | -365.5 | |
| 0.00 | 0.90 | 0.00 | 0.56 | 18.29 | 131.47 | 36.12 | 291.77 | 0.6049 | -624.0 | -476.9 | |
| 0.00 | 1.62 | 0.00 | 0.96 | 10.87 | 128.18 | 32.83 | 279.86 | 0.5425 | 633.0 | 546.1 | |
| 0.00 | 0.99 | 0.00 | 0.58 | 12.73 | 127.84 | 32.49 | 283.35 | 0.5406 | 730.0 | 624.4 | |
| 0.00 | 1.26 | 0.00 | 0.73 | 9.95 | 126.22 | 30.86 | 278.39 | 0.5128 | 552.0 | 555.0 | |
| 0.00 | 0.99 | 0.00 | 0.57 | 9.85 | 125.95 | 30.60 | 278.22 | 0.5088 | 547.0 | 480.2 | |
| 1.17 | 26.25 | 0.67 | 15.02 | 10.51 | 125.59 | 30.24 | 279.58 | 0.5042 | 761.6 | 621.3 | |
| 0.54 | 2.26 | 0.31 | 1.29 | 9.57 | 125.50 | 30.14 | 277.72 | 0.5017 | 908.2 | 763.4 | |
| 14.07 | -9.00 | 8.05 | -9.00 | 10.12 | 125.44 | 30.09 | 278.83 | 0.5015 | 1011.2 | 999999 | |
| 0.00 | 1.62 | 0.00 | 0.93 | 10.91 | 125.50 | 30.14 | 280.40 | 0.5033 | 732.0 | 569.5 | |
| 0.00 | 2.07 | 0.00 | 1.18 | 9.17 | 124.96 | 29.61 | 276.98 | 0.4933 | 845.0 | 702.2 | |
| 0.00 | 0.63 | 0.00 | 0.35 | 9.06 | 123.19 | 27.84 | 276.93 | 0.4665 | -614.0 | -525.0 | |
| 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. | |