| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 55.55 | 334.83 | 29.63 | 178.88 | 17.94 | 60.98 | -2.63 | 6.56 | 0.3758 | -701.9 | -344.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.56 | 304.57 | 23.74 | 162.33 | 17.69 | 61.61 | -2.00 | 5.17 | 0.3699 | -1424.8 | -443.9 | |
| 3.93 | -1.00 | 2.10 | -1.00 | 18.18 | 61.16 | -2.45 | 6.18 | 0.3785 | -936.7 | 999999 | |
| 3.13 | -1.00 | 1.67 | -1.00 | 17.92 | 61.00 | -2.60 | 6.65 | 0.3746 | -1020.0 | 999999 | |
| 0.27 | -1.00 | 0.14 | -1.00 | 18.08 | 60.91 | -2.70 | 6.84 | 0.3774 | -733.0 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.59 | 20.85 | 59.99 | -3.62 | 8.05 | 0.4234 | -711.0 | -555.7 | |
| 1.70 | 2.14 | 0.92 | 1.16 | 18.53 | 57.00 | -6.61 | 16.02 | 0.3971 | 910.3 | 854.2 | |
| 0.00 | 2.68 | 0.00 | 1.45 | 18.79 | 56.92 | -6.68 | 16.00 | 0.4014 | 734.0 | 629.0 | |
| 0.00 | 4.11 | 0.00 | 2.21 | 18.30 | 56.49 | -7.11 | 17.35 | 0.3959 | 640.0 | 672.5 | |
| 0.00 | 3.39 | 0.00 | 1.91 | 23.20 | 55.89 | -7.71 | 15.21 | 0.4723 | 671.0 | 585.4 | |
| 1.16 | 3.30 | 0.62 | 1.78 | 18.01 | 56.12 | -7.49 | 18.44 | 0.3934 | -484.7 | 117.5 | |
| 0.00 | 1.07 | 0.00 | 0.58 | 18.96 | 55.95 | -7.66 | 18.04 | 0.4086 | 826.0 | 707.7 | |
| 0.00 | 1.88 | 0.00 | 1.02 | 19.32 | 55.87 | -7.74 | 17.93 | 0.4145 | 612.0 | 544.3 | |
| 0.00 | 1.52 | 0.00 | 0.86 | 23.64 | 55.43 | -8.17 | 15.78 | 0.4808 | 689.0 | 519.5 | |
| 0.00 | 0.71 | 0.00 | 0.40 | 23.37 | 55.25 | -8.36 | 16.29 | 0.4776 | 679.0 | 568.6 | |
| 0.00 | 0.98 | 0.00 | 0.56 | 23.42 | 53.81 | -9.79 | 18.85 | 0.4850 | 749.0 | 541.3 | |
| 0.80 | 4.55 | 0.44 | 2.47 | 18.52 | 54.00 | -9.60 | 22.63 | 0.4129 | 857.3 | 881.1 | |
| 0.00 | 1.25 | 0.00 | 0.68 | 18.79 | 53.40 | -10.20 | 23.60 | 0.4205 | 1019.0 | 849.7 | |
| 0.00 | 1.61 | 0.00 | 0.88 | 19.09 | 53.06 | -10.55 | 24.00 | 0.4270 | 729.0 | 569.7 | |
| 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. | |