| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.94 | 134.65 | 14.44 | 91.76 | 16.61 | 27.84 | 43.16 | 286.97 | 0.6872 | -424.1 | -204.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.02 | 113.78 | 9.67 | 78.56 | 16.33 | 28.78 | 44.10 | 286.34 | 0.6983 | -1030.9 | -294.8 | |
| 5.93 | -1.00 | 4.09 | -1.00 | 16.59 | 28.63 | 43.96 | 286.74 | 0.6970 | -1016.9 | 999999 | |
| 0.99 | -1.00 | 0.68 | -1.00 | 16.40 | 28.31 | 43.64 | 286.52 | 0.6929 | -1025.5 | 999999 | |
| 0.00 | 1.17 | 0.00 | 0.79 | 18.16 | 26.91 | 42.24 | 289.36 | 0.6793 | -593.0 | -445.9 | |
| 0.00 | 0.72 | 0.00 | 0.48 | 17.63 | 26.62 | 41.95 | 288.64 | 0.6747 | -557.0 | -565.6 | |
| 0.00 | 1.62 | 0.00 | 1.08 | 18.00 | 26.61 | 41.93 | 289.20 | 0.6753 | -616.0 | -560.9 | |
| 0.00 | 1.44 | 0.00 | 0.96 | 17.62 | 26.36 | 41.69 | 288.69 | 0.6715 | -735.0 | -592.0 | |
| 0.00 | 0.81 | 0.00 | 0.53 | 17.04 | 25.78 | 41.11 | 287.97 | 0.6631 | -583.0 | -461.1 | |
| 0.00 | 2.34 | 0.00 | 1.46 | 17.02 | 21.84 | 37.17 | 288.97 | 0.6131 | 487.0 | 416.2 | |
| 0.00 | 1.98 | 0.00 | 1.24 | 17.61 | 21.94 | 37.27 | 289.87 | 0.6159 | 564.0 | 502.3 | |
| 0.00 | 1.17 | 0.00 | 0.72 | 16.83 | 21.00 | 36.33 | 288.92 | 0.6016 | 698.0 | 566.6 | |
| 0.00 | 0.99 | 0.00 | 0.62 | 18.71 | 21.29 | 36.62 | 291.86 | 0.6110 | 535.0 | 434.4 | |
| 0.00 | 3.95 | 0.00 | 2.45 | 18.31 | 20.83 | 36.16 | 291.37 | 0.6038 | 743.0 | 612.9 | |
| 0.00 | 1.35 | 0.00 | 0.83 | 17.97 | 20.71 | 36.04 | 290.87 | 0.6012 | 763.0 | 607.5 | |
| 0.00 | 0.99 | 0.00 | 0.61 | 18.99 | 20.49 | 35.81 | 292.60 | 0.6016 | 696.0 | 609.0 | |
| 0.00 | 1.26 | 0.00 | 0.77 | 17.22 | 19.99 | 35.32 | 289.88 | 0.5894 | 758.0 | 613.4 | |
| 0.00 | 1.08 | 0.00 | 0.66 | 17.64 | 20.09 | 35.41 | 290.55 | 0.5920 | 603.0 | 511.3 | |
| 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. | |