| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.91 | 39.67 | 7.37 | 21.22 | -17.42 | 98.17 | -1.95 | 175.80 | 0.3791 | -89.0 | -327.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.89 | 15.21 | 5.77 | 8.06 | -16.41 | 103.87 | 3.75 | 190.15 | 0.3579 | 1019.4 | 704.7 | |
| 3.02 | 4.93 | 1.60 | 2.61 | -16.85 | 100.40 | 0.28 | 180.75 | 0.3596 | 1108.6 | 790.5 | |
| 0.00 | 1.21 | 0.00 | 0.64 | -17.04 | 95.76 | -4.36 | 168.63 | 0.3698 | -962.0 | -768.9 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -17.27 | 94.47 | -5.64 | 165.56 | 0.3782 | -947.0 | -822.6 | |
| 0.00 | 1.47 | 0.00 | 0.79 | -17.47 | 94.34 | -5.77 | 165.37 | 0.3817 | -847.0 | -680.5 | |
| 0.00 | 3.20 | 0.00 | 1.72 | -17.66 | 94.15 | -5.97 | 165.04 | 0.3855 | -805.0 | -695.3 | |
| 0.00 | 2.16 | 0.00 | 1.16 | -18.18 | 93.85 | -6.27 | 164.69 | 0.3948 | -758.0 | -692.6 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -17.50 | 93.65 | -6.47 | 163.74 | 0.3852 | -876.0 | -725.4 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -17.09 | 93.60 | -6.51 | 163.30 | 0.3790 | -807.0 | -670.6 | |
| 0.00 | 1.12 | 0.00 | 0.60 | -17.31 | 93.53 | -6.58 | 163.31 | 0.3828 | -860.0 | -751.3 | |
| 0.00 | 1.56 | 0.00 | 0.84 | -18.11 | 93.38 | -6.74 | 163.56 | 0.3959 | -782.0 | -707.7 | |
| 0.00 | 0.60 | 0.00 | 0.33 | -20.76 | 91.43 | -8.68 | 161.42 | 0.4451 | -796.0 | -673.6 | |
| 0.00 | 2.85 | 0.00 | 1.56 | -19.75 | 91.27 | -8.85 | 160.28 | 0.4310 | -769.0 | -613.3 | |
| 0.00 | 1.99 | 0.00 | 1.10 | -20.70 | 91.02 | -9.10 | 160.56 | 0.4463 | -171.0 | -320.2 | |
| 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. | |