| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.59 | 26.41 | 4.84 | 18.29 | -10.35 | 83.09 | 43.37 | 256.01 | 0.6970 | -49.5 | -52.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.54 | 0.00 | 0.40 | -11.66 | 87.43 | 47.71 | 255.34 | 0.7511 | 502.0 | 437.8 | |
| 3.97 | 11.91 | 2.92 | 8.75 | -9.59 | 86.92 | 47.20 | 257.99 | 0.7419 | 656.5 | 568.7 | |
| 2.26 | -2.00 | 1.66 | -2.00 | -9.72 | 86.76 | 47.04 | 257.79 | 0.7403 | 869.3 | 999999 | |
| 0.00 | 0.36 | 0.00 | 0.26 | -10.02 | 84.98 | 45.26 | 257.05 | 0.7200 | 312.0 | 357.2 | |
| 0.36 | 2.08 | 0.26 | 1.47 | -13.00 | 84.18 | 44.46 | 252.76 | 0.7168 | 598.2 | 478.5 | |
| 0.00 | 1.71 | 0.00 | 1.14 | -10.37 | 81.08 | 41.36 | 255.67 | 0.6731 | -661.0 | -561.3 | |
| 0.00 | 0.90 | 0.00 | 0.60 | -10.16 | 80.92 | 41.20 | 255.95 | 0.6707 | -531.0 | -421.8 | |
| 0.00 | 1.35 | 0.00 | 0.89 | -10.44 | 80.07 | 40.35 | 255.30 | 0.6605 | -699.0 | -604.9 | |
| 0.00 | 1.53 | 0.00 | 0.97 | -5.72 | 77.66 | 37.94 | 262.11 | 0.6198 | -538.0 | -366.2 | |
| 0.00 | 1.26 | 0.00 | 0.81 | -11.14 | 78.09 | 38.37 | 253.65 | 0.6369 | -691.0 | -620.0 | |
| 0.00 | 0.99 | 0.00 | 0.63 | -9.70 | 77.49 | 37.77 | 255.71 | 0.6252 | -722.0 | -615.5 | |
| 0.00 | 1.89 | 0.00 | 1.20 | -10.60 | 77.50 | 37.77 | 254.31 | 0.6277 | -665.0 | -525.8 | |
| 0.00 | 1.26 | 0.00 | 0.78 | -14.23 | 74.14 | 34.42 | 247.18 | 0.5966 | -620.0 | -524.0 | |
| 0.00 | 0.63 | 0.00 | 0.39 | -17.51 | 72.86 | 33.13 | 241.27 | 0.5966 | -634.0 | -549.1 | |
| 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. | |