| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.60 | 42.78 | 2.94 | 22.53 | 17.52 | 40.44 | -7.29 | 13.18 | 0.3423 | 92.7 | 118.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.18 | 0.00 | 0.62 | 20.48 | 47.81 | 0.09 | 359.77 | 0.3606 | 741.0 | 642.2 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 20.38 | 47.65 | -0.08 | 0.20 | 0.3590 | 822.0 | 676.5 | |
| 0.00 | 1.72 | 0.00 | 0.91 | 20.41 | 46.48 | -1.24 | 3.25 | 0.3601 | 909.0 | 693.1 | |
| 5.60 | 12.57 | 2.94 | 6.58 | 18.18 | 44.61 | -3.12 | 9.13 | 0.3269 | -1088.8 | -701.6 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 17.60 | 44.04 | -3.68 | 11.10 | 0.3192 | -1062.0 | -901.2 | |
| 0.00 | 2.62 | 0.00 | 1.36 | 16.20 | 41.81 | -5.91 | 18.92 | 0.3063 | -760.0 | -622.8 | |
| 0.00 | 2.44 | 0.00 | 1.27 | 15.70 | 41.10 | -6.62 | 21.64 | 0.3025 | -1052.0 | -861.7 | |
| 0.00 | 1.63 | 0.00 | 0.85 | 16.24 | 40.67 | -7.06 | 22.20 | 0.3135 | -641.0 | -517.3 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 16.75 | 37.27 | -10.45 | 30.27 | 0.3460 | 866.0 | 667.2 | |
| 0.00 | 1.72 | 0.00 | 0.90 | 15.55 | 36.73 | -11.00 | 33.53 | 0.3342 | 1032.0 | 756.1 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 16.18 | 36.40 | -11.32 | 33.21 | 0.3457 | 1116.0 | 905.3 | |
| 0.00 | 0.81 | 0.00 | 0.43 | 16.72 | 36.08 | -11.65 | 33.06 | 0.3559 | 677.0 | 568.6 | |
| 0.00 | 1.99 | 0.00 | 1.07 | 18.94 | 35.70 | -12.02 | 30.57 | 0.3891 | 872.0 | 559.0 | |
| 0.00 | 7.59 | 0.00 | 4.04 | 17.14 | 35.37 | -12.35 | 33.93 | 0.3679 | 423.0 | 762.2 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 17.43 | 35.25 | -12.47 | 33.72 | 0.3727 | 641.0 | 550.4 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 17.24 | 35.00 | -12.72 | 34.54 | 0.3725 | 979.0 | 771.9 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 14.83 | 33.80 | -13.92 | 41.25 | 0.3542 | -607.0 | -461.4 | |
| 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. | |