| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.12 | 0.00 | 9.02 | -19.58 | 73.96 | 7.98 | 197.85 | 0.4629 | 316.4 | 295.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.96 | 0.00 | 0.56 | -20.81 | 80.86 | 14.88 | 208.00 | 0.5133 | 656.0 | 619.1 | |
| 0.00 | 1.31 | 0.00 | 0.72 | -14.71 | 79.55 | 13.58 | 212.63 | 0.4229 | 587.0 | 510.7 | |
| 0.00 | 1.58 | 0.00 | 0.86 | -15.11 | 77.83 | 11.85 | 208.72 | 0.4144 | 869.0 | 675.8 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -17.38 | 76.43 | 10.46 | 203.46 | 0.4368 | 679.0 | 548.9 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -17.40 | 75.92 | 9.95 | 202.42 | 0.4340 | 737.0 | 620.7 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -16.48 | 75.52 | 9.55 | 202.46 | 0.4182 | 656.0 | 477.5 | |
| 0.00 | 1.23 | 0.00 | 0.67 | -16.93 | 75.29 | 9.32 | 201.55 | 0.4234 | 732.0 | 638.5 | |
| 0.00 | 1.14 | 0.00 | 0.63 | -18.86 | 74.79 | 8.81 | 198.91 | 0.4490 | 706.0 | 588.8 | |
| 0.00 | 1.31 | 0.00 | 0.73 | -18.79 | 74.53 | 8.55 | 198.45 | 0.4467 | 765.0 | 602.7 | |
| 0.00 | 1.84 | 0.00 | 1.01 | -18.22 | 74.31 | 8.33 | 198.43 | 0.4372 | 783.0 | 618.2 | |
| 0.00 | 0.96 | 0.00 | 0.55 | -23.85 | 68.63 | 2.66 | 184.84 | 0.5052 | -732.0 | -566.5 | |
| 0.00 | 1.05 | 0.00 | 0.60 | -23.67 | 67.52 | 1.54 | 182.83 | 0.5013 | -719.0 | -634.3 | |
| 0.00 | 1.05 | 0.00 | 0.63 | -27.56 | 67.57 | 1.59 | 182.53 | 0.5590 | -622.0 | -477.8 | |
| 0.00 | 0.88 | 0.00 | 0.53 | -28.79 | 63.41 | -2.56 | 176.09 | 0.5775 | -667.0 | -621.9 | |
| 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. | |