| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.46 | 37.60 | 9.83 | 25.68 | 8.61 | 3.91 | 43.34 | 279.44 | 0.6900 | -105.4 | -154.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.61 | 8.40 | 6.00 | 45.43 | 278.89 | 0.7157 | -345.0 | -302.6 | |
| 0.00 | 0.26 | 0.00 | 0.18 | 7.90 | 5.80 | 45.23 | 278.21 | 0.7128 | -433.0 | -444.0 | |
| 6.37 | 9.98 | 4.47 | 7.01 | 8.12 | 5.66 | 45.09 | 278.52 | 0.7113 | -891.0 | -543.7 | |
| 0.00 | 0.77 | 0.00 | 0.54 | 8.47 | 5.67 | 45.10 | 279.02 | 0.7117 | -556.0 | -475.6 | |
| 0.43 | 5.08 | 0.30 | 3.54 | 8.11 | 5.02 | 44.45 | 278.57 | 0.7035 | -887.0 | -691.2 | |
| 0.00 | 0.69 | 0.00 | 0.48 | 8.12 | 4.81 | 44.24 | 278.61 | 0.7009 | -653.0 | -592.4 | |
| 0.00 | 2.84 | 0.00 | 1.96 | 8.13 | 4.52 | 43.95 | 278.65 | 0.6973 | -790.0 | -702.8 | |
| 0.00 | 0.60 | 0.00 | 0.41 | 8.58 | 4.29 | 43.72 | 279.33 | 0.6950 | -295.0 | -311.6 | |
| 0.00 | 1.55 | 0.00 | 1.04 | 9.75 | 2.74 | 42.17 | 281.24 | 0.6769 | 574.0 | 467.2 | |
| 0.00 | 1.46 | 0.00 | 0.97 | 10.15 | 2.23 | 41.67 | 281.93 | 0.6712 | 835.0 | 718.9 | |
| 0.00 | 1.29 | 0.00 | 0.86 | 10.30 | 2.18 | 41.61 | 282.17 | 0.6707 | 654.0 | 509.3 | |
| 6.63 | 9.47 | 4.38 | 6.26 | 8.73 | 1.90 | 41.33 | 279.85 | 0.6649 | 803.4 | 574.1 | |
| 1.03 | 2.75 | 0.68 | 1.82 | 9.63 | 1.87 | 41.30 | 281.21 | 0.6657 | 788.3 | 689.0 | |
| 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. | |