| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.06 | 72.55 | 19.70 | 52.87 | 17.04 | 19.66 | 44.70 | 293.54 | 0.7353 | -326.7 | -323.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.42 | 24.16 | 4.84 | 18.15 | 16.95 | 21.55 | 46.60 | 292.69 | 0.7556 | -568.2 | -285.4 | |
| 3.53 | -1.00 | 2.64 | -1.00 | 17.04 | 21.07 | 46.12 | 292.97 | 0.7508 | -679.0 | 999999 | |
| 4.80 | 27.23 | 3.56 | 20.11 | 16.69 | 20.83 | 45.87 | 292.61 | 0.7470 | -721.2 | -533.7 | |
| 0.00 | 0.54 | 0.00 | 0.40 | 17.11 | 20.64 | 45.68 | 293.21 | 0.7463 | -686.0 | -594.5 | |
| 4.34 | -3.00 | 3.20 | -3.00 | 16.69 | 20.46 | 45.51 | 292.73 | 0.7431 | -906.7 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.46 | 17.52 | 19.86 | 44.90 | 294.03 | 0.7393 | -592.0 | -508.1 | |
| 1.63 | 5.52 | 1.15 | 3.87 | 16.95 | 17.56 | 42.61 | 294.16 | 0.7120 | -740.9 | -609.1 | |
| 0.00 | 1.45 | 0.00 | 1.01 | 17.04 | 16.94 | 41.99 | 294.54 | 0.7054 | -879.0 | -678.5 | |
| 0.00 | 0.81 | 0.00 | 0.55 | 16.53 | 14.95 | 39.99 | 294.71 | 0.6805 | 608.0 | 510.3 | |
| 0.00 | 1.09 | 0.00 | 0.74 | 17.52 | 15.16 | 40.21 | 295.98 | 0.6871 | 476.0 | 406.9 | |
| 1.36 | 8.14 | 0.92 | 5.54 | 17.74 | 15.01 | 40.06 | 296.36 | 0.6864 | 696.3 | 502.9 | |
| 3.53 | -11.00 | 2.40 | -11.00 | 17.97 | 15.03 | 40.08 | 296.66 | 0.6876 | 724.7 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.55 | 18.19 | 14.93 | 39.97 | 297.01 | 0.6873 | 573.0 | 498.3 | |
| 1.45 | 2.17 | 0.99 | 1.49 | 18.96 | 15.06 | 40.11 | 298.00 | 0.6923 | 594.9 | 559.8 | |
| 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. | |