| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 26.60 | 0.00 | 14.15 | -13.51 | 255.89 | 12.92 | 216.50 | 0.3662 | 433.8 | 501.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.82 | 0.00 | 0.44 | -13.16 | 259.79 | 16.81 | 224.79 | 0.4015 | 688.0 | 536.1 | |
| 0.00 | 0.64 | 0.00 | 0.34 | -13.69 | 259.33 | 16.36 | 223.07 | 0.4024 | 726.0 | 584.9 | |
| 0.00 | 1.27 | 0.00 | 0.68 | -13.30 | 258.88 | 15.91 | 222.97 | 0.3930 | 807.0 | 586.2 | |
| 0.00 | 1.45 | 0.00 | 0.79 | -14.35 | 258.79 | 15.82 | 220.99 | 0.4043 | 558.0 | 488.4 | |
| 0.00 | 1.63 | 0.00 | 0.88 | -14.16 | 258.71 | 15.74 | 221.18 | 0.4012 | 799.0 | 592.7 | |
| 0.00 | 1.54 | 0.00 | 0.83 | -14.03 | 258.51 | 15.53 | 221.03 | 0.3975 | 971.0 | 770.1 | |
| 0.00 | 1.09 | 0.00 | 0.58 | -12.99 | 257.66 | 14.69 | 221.27 | 0.3762 | 821.0 | 624.2 | |
| 0.00 | 5.36 | 0.00 | 2.83 | -11.83 | 256.22 | 13.24 | 220.52 | 0.3466 | 593.0 | 689.2 | |
| 0.00 | 6.36 | 0.00 | 3.40 | -14.68 | 255.63 | 12.66 | 214.35 | 0.3773 | 941.0 | 806.5 | |
| 0.00 | 1.54 | 0.00 | 0.81 | -11.99 | 254.31 | 11.34 | 215.92 | 0.3292 | 858.0 | 672.4 | |
| 0.00 | 1.36 | 0.00 | 0.72 | -14.44 | 251.80 | 8.83 | 205.85 | 0.3425 | -853.0 | -657.5 | |
| 0.00 | 1.27 | 0.00 | 0.67 | -14.73 | 251.59 | 8.62 | 204.94 | 0.3452 | -885.0 | -651.2 | |
| 0.00 | 1.09 | 0.00 | 0.56 | -11.26 | 251.19 | 8.22 | 208.93 | 0.2911 | 820.0 | 634.8 | |
| 0.00 | 1.18 | 0.00 | 0.62 | -14.62 | 250.76 | 7.79 | 202.92 | 0.3381 | -771.0 | -545.5 | |
| 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. | |