| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.40 | 64.71 | 11.09 | 36.59 | 8.25 | 133.73 | -24.08 | 57.28 | 0.4797 | 253.6 | 213.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.10 | 0.00 | 1.65 | 7.22 | 142.24 | -15.57 | 47.46 | 0.3630 | -754.0 | -639.7 | |
| 0.00 | 1.21 | 0.00 | 0.64 | 7.43 | 142.23 | -15.58 | 47.04 | 0.3655 | -884.0 | -688.8 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 7.38 | 141.79 | -16.01 | 47.92 | 0.3702 | -580.0 | -563.1 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 6.34 | 140.99 | -16.82 | 51.48 | 0.3691 | -858.0 | -676.8 | |
| 0.00 | 0.78 | 0.00 | 0.41 | 5.91 | 140.47 | -17.34 | 53.28 | 0.3714 | -880.0 | -731.0 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 5.97 | 139.65 | -18.15 | 54.42 | 0.3826 | -717.0 | -501.9 | |
| 0.00 | 3.71 | 0.00 | 1.99 | 6.65 | 139.47 | -18.33 | 53.28 | 0.3915 | -981.0 | -760.0 | |
| 0.00 | 1.81 | 0.00 | 0.97 | 6.14 | 139.30 | -18.50 | 54.60 | 0.3888 | -852.0 | -668.0 | |
| 0.00 | 0.86 | 0.00 | 0.49 | 7.36 | 133.06 | -24.74 | 59.97 | 0.4814 | 499.0 | 410.0 | |
| 11.38 | 15.60 | 6.48 | 8.88 | 8.79 | 132.84 | -24.97 | 57.69 | 0.4956 | 957.1 | 553.7 | |
| 0.00 | 2.67 | 0.00 | 1.53 | 8.55 | 132.02 | -25.78 | 58.93 | 0.5042 | 867.0 | 717.3 | |
| 5.95 | 26.97 | 3.42 | 15.52 | 8.49 | 131.63 | -26.18 | 59.44 | 0.5088 | 968.1 | 654.4 | |
| 0.00 | 0.69 | 0.00 | 0.40 | 9.29 | 131.50 | -26.31 | 58.21 | 0.5167 | 471.0 | 282.2 | |
| 0.00 | 1.72 | 0.00 | 1.00 | 9.93 | 131.28 | -26.53 | 57.39 | 0.5244 | 757.0 | 583.8 | |
| 0.00 | 1.29 | 0.00 | 0.75 | 8.72 | 131.38 | -26.43 | 59.30 | 0.5138 | 456.0 | 436.7 | |
| 1.12 | -12.00 | 0.64 | -12.00 | 8.13 | 131.32 | -26.49 | 60.34 | 0.5102 | 861.8 | 999999 | |
| 0.95 | -12.00 | 0.55 | -12.00 | 8.29 | 131.31 | -26.50 | 60.09 | 0.5115 | 846.6 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.61 | 11.10 | 130.90 | -26.91 | 55.90 | 0.5385 | -711.0 | -620.2 | |
| 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. | |