| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.97 | 0.00 | 11.23 | -18.75 | 159.57 | -12.91 | 153.41 | 0.4727 | 662.4 | 570.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.08 | 0.00 | 1.14 | -17.34 | 164.55 | -7.93 | 161.75 | 0.4224 | 773.0 | 671.0 | |
| 0.00 | 0.81 | 0.00 | 0.45 | -17.52 | 160.59 | -11.89 | 153.89 | 0.4484 | 756.0 | 613.7 | |
| 0.00 | 1.72 | 0.00 | 0.97 | -19.88 | 159.89 | -12.60 | 154.92 | 0.4857 | 941.0 | 729.5 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -20.91 | 159.50 | -12.98 | 155.20 | 0.5022 | 741.0 | 648.0 | |
| 0.00 | 2.62 | 0.00 | 1.46 | -17.50 | 159.75 | -12.74 | 152.29 | 0.4542 | 876.0 | 720.0 | |
| 0.00 | 2.26 | 0.00 | 1.25 | -17.31 | 159.60 | -12.89 | 151.81 | 0.4526 | 916.0 | 778.7 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -21.09 | 159.29 | -13.20 | 154.99 | 0.5060 | 696.0 | 524.3 | |
| 0.00 | 1.99 | 0.00 | 1.10 | -17.08 | 159.42 | -13.07 | 151.22 | 0.4508 | 915.0 | 725.9 | |
| 0.00 | 1.54 | 0.00 | 0.86 | -18.22 | 159.23 | -13.25 | 152.12 | 0.4675 | 821.0 | 645.5 | |
| 0.00 | 0.72 | 0.00 | 0.41 | -20.96 | 159.00 | -13.49 | 154.40 | 0.5061 | 550.0 | 494.6 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -21.27 | 158.90 | -13.59 | 154.52 | 0.5109 | 561.0 | 460.1 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -17.05 | 159.16 | -13.33 | 150.72 | 0.4524 | 783.0 | 644.8 | |
| 0.00 | 0.72 | 0.00 | 0.42 | -20.80 | 157.40 | -15.09 | 151.68 | 0.5148 | 668.0 | 569.4 | |
| 0.00 | 1.45 | 0.00 | 0.86 | -21.85 | 154.55 | -17.94 | 148.49 | 0.5490 | -724.0 | -589.2 | |
| 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. | |