| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.80 | 51.77 | 9.99 | 26.30 | 15.05 | 24.95 | -1.67 | 7.11 | 0.2166 | -19.4 | -139.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.91 | 0.00 | 0.99 | 19.06 | 29.99 | 3.37 | 348.78 | 0.2865 | -818.0 | -654.0 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 17.14 | 28.17 | 1.54 | 354.06 | 0.2498 | -831.0 | -580.8 | |
| 13.44 | 19.80 | 6.77 | 9.97 | 13.24 | 26.26 | -0.36 | 1.96 | 0.1818 | 1081.3 | 742.4 | |
| 0.00 | 2.45 | 0.00 | 1.25 | 15.45 | 25.12 | -1.51 | 6.61 | 0.2211 | -1033.0 | -809.1 | |
| 3.09 | 4.00 | 1.57 | 2.04 | 16.32 | 24.57 | -2.05 | 8.37 | 0.2371 | -905.3 | -808.7 | |
| 1.73 | 2.72 | 0.87 | 1.38 | 14.32 | 24.53 | -2.10 | 10.07 | 0.2035 | -883.8 | -757.3 | |
| 0.00 | 1.63 | 0.00 | 0.83 | 15.79 | 24.33 | -2.30 | 9.76 | 0.2288 | -1048.0 | -775.6 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 16.67 | 24.25 | -2.37 | 9.41 | 0.2437 | -713.0 | -542.5 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 13.42 | 24.19 | -2.43 | 12.64 | 0.1895 | 870.0 | 687.2 | |
| 0.00 | 0.73 | 0.00 | 0.37 | 14.57 | 24.02 | -2.60 | 12.17 | 0.2094 | -707.0 | -519.9 | |
| 1.54 | 2.36 | 0.78 | 1.20 | 15.23 | 23.89 | -2.74 | 12.10 | 0.2208 | -974.3 | -724.0 | |
| 0.00 | 3.00 | 0.00 | 1.52 | 14.98 | 23.86 | -2.76 | 12.47 | 0.2167 | -926.0 | -870.4 | |
| 0.00 | 1.91 | 0.00 | 0.97 | 14.97 | 23.51 | -3.11 | 13.98 | 0.2181 | -772.0 | -579.0 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 17.39 | 23.03 | -3.60 | 13.39 | 0.2598 | -772.0 | -553.5 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 17.38 | 22.80 | -3.82 | 14.19 | 0.2607 | -857.0 | -741.3 | |
| 0.00 | 2.18 | 0.00 | 1.12 | 18.01 | 21.76 | -4.86 | 17.09 | 0.2756 | 864.0 | 642.4 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 17.19 | 20.79 | -5.83 | 21.35 | 0.2679 | 918.0 | 712.2 | |
| 0.00 | 2.09 | 0.00 | 1.08 | 17.57 | 20.78 | -5.85 | 20.86 | 0.2739 | 990.0 | 750.9 | |
| 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. | |