| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.69 | 37.08 | 6.74 | 19.70 | 24.49 | 78.47 | 8.34 | 338.11 | 0.3616 | -428.1 | -239.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.34 | 6.98 | 3.37 | 3.71 | 23.50 | 81.24 | 11.11 | 330.77 | 0.3635 | -827.4 | -772.5 | |
| 3.99 | 5.26 | 2.12 | 2.79 | 23.51 | 80.74 | 10.61 | 331.88 | 0.3596 | -943.0 | -699.8 | |
| 2.36 | 2.99 | 1.25 | 1.59 | 23.58 | 80.27 | 10.14 | 333.02 | 0.3571 | -872.1 | -831.4 | |
| 0.00 | 3.08 | 0.00 | 1.62 | 22.53 | 79.79 | 9.66 | 332.63 | 0.3385 | -861.0 | -544.3 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 23.31 | 79.17 | 9.04 | 335.18 | 0.3453 | -776.0 | -599.9 | |
| 0.00 | 1.90 | 0.00 | 1.00 | 23.08 | 79.02 | 8.89 | 335.24 | 0.3410 | -979.0 | -796.5 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 23.76 | 78.93 | 8.80 | 336.33 | 0.3504 | -892.0 | -672.2 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 27.02 | 77.56 | 7.43 | 342.83 | 0.3917 | -939.0 | -726.0 | |
| 0.00 | 3.99 | 0.00 | 2.12 | 25.01 | 77.19 | 7.06 | 341.85 | 0.3591 | -953.0 | -759.2 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 25.59 | 77.12 | 6.99 | 342.55 | 0.3677 | -801.0 | -573.3 | |
| 0.00 | 1.63 | 0.00 | 0.88 | 27.48 | 74.82 | 4.69 | 349.17 | 0.3881 | 647.0 | 561.4 | |
| 0.00 | 1.63 | 0.00 | 0.88 | 27.28 | 74.82 | 4.69 | 349.08 | 0.3850 | 794.0 | 660.9 | |
| 0.00 | 2.81 | 0.00 | 1.50 | 26.72 | 74.38 | 4.25 | 349.78 | 0.3749 | 885.0 | 656.5 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 26.57 | 73.29 | 3.16 | 352.31 | 0.3696 | 784.0 | 660.1 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 24.74 | 73.17 | 3.04 | 351.82 | 0.3398 | 946.0 | 722.2 | |
| 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. | |