| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.60 | 52.46 | 3.97 | 27.50 | 17.16 | 40.63 | -6.00 | 17.65 | 0.3283 | 21.0 | -3.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 0.71 | 17.46 | 48.66 | 2.03 | 353.76 | 0.3124 | 837.0 | 635.7 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 15.74 | 47.44 | 0.81 | 357.22 | 0.2821 | 815.0 | 716.5 | |
| 0.00 | 0.81 | 0.00 | 0.43 | 20.43 | 46.55 | -0.07 | 0.20 | 0.3596 | 707.0 | 607.9 | |
| 5.70 | 13.29 | 2.98 | 6.96 | 18.23 | 44.70 | -1.93 | 5.68 | 0.3249 | -1023.3 | -770.3 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 18.52 | 44.69 | -1.93 | 5.59 | 0.3297 | -472.0 | -399.5 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 17.68 | 44.19 | -2.44 | 7.37 | 0.3169 | -790.0 | -655.0 | |
| 0.00 | 6.60 | 0.00 | 3.42 | 15.77 | 41.08 | -5.55 | 18.31 | 0.2974 | -736.0 | -833.9 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 15.84 | 40.86 | -5.77 | 18.92 | 0.2996 | -947.0 | -832.9 | |
| 1.90 | 4.43 | 0.99 | 2.30 | 16.19 | 40.81 | -5.81 | 18.66 | 0.3053 | -900.7 | -742.0 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 15.68 | 40.70 | -5.92 | 19.58 | 0.2979 | -872.0 | -665.8 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 17.47 | 37.72 | -8.91 | 25.53 | 0.3441 | 910.0 | 650.2 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 16.70 | 37.28 | -9.35 | 27.70 | 0.3363 | 892.0 | 704.4 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 15.53 | 36.72 | -9.90 | 30.90 | 0.3240 | 823.0 | 658.5 | |
| 0.00 | 1.81 | 0.00 | 0.95 | 16.22 | 36.37 | -10.26 | 30.66 | 0.3368 | 1034.0 | 763.5 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 18.98 | 35.68 | -10.94 | 28.25 | 0.3810 | 828.0 | 684.2 | |
| 0.00 | 10.13 | 0.00 | 5.37 | 17.18 | 35.34 | -11.28 | 31.55 | 0.3588 | 564.0 | 762.4 | |
| 0.00 | 1.81 | 0.00 | 0.96 | 17.34 | 34.98 | -11.65 | 32.12 | 0.3641 | 746.0 | 530.3 | |
| 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. | |