| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.64 | 41.98 | 7.65 | 23.77 | -18.05 | 78.09 | -22.78 | 130.62 | 0.4863 | -27.8 | -270.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.44 | 11.09 | 4.68 | 6.15 | -17.67 | 80.73 | -20.14 | 133.23 | 0.4522 | 966.8 | 718.9 | |
| 0.00 | 2.39 | 0.00 | 1.34 | -17.42 | 79.23 | -21.64 | 130.86 | 0.4672 | 814.0 | 628.2 | |
| 0.00 | 0.94 | 0.00 | 0.53 | -17.11 | 78.70 | -22.17 | 129.69 | 0.4705 | 733.0 | 672.6 | |
| 0.68 | 3.75 | 0.38 | 2.11 | -17.24 | 78.25 | -22.62 | 129.36 | 0.4770 | 1080.8 | 796.9 | |
| 0.00 | 1.71 | 0.00 | 0.97 | -18.77 | 77.80 | -23.06 | 131.36 | 0.4962 | -663.0 | -549.9 | |
| 0.00 | 4.01 | 0.00 | 2.29 | -18.36 | 77.39 | -23.48 | 130.23 | 0.4973 | -841.0 | -726.8 | |
| 1.71 | 12.20 | 0.98 | 7.00 | -18.61 | 76.94 | -23.93 | 130.13 | 0.5047 | -876.5 | -763.5 | |
| 2.13 | -7.00 | 1.22 | -7.00 | -18.52 | 76.72 | -24.15 | 129.73 | 0.5065 | -987.8 | 999999 | |
| 0.68 | -7.00 | 0.39 | -7.00 | -18.74 | 76.58 | -24.29 | 129.93 | 0.5100 | -774.6 | 999999 | |
| 0.00 | 1.79 | 0.00 | 1.02 | -17.80 | 76.72 | -24.15 | 128.57 | 0.5002 | -1047.0 | -819.3 | |
| 0.00 | 0.68 | 0.00 | 0.39 | -18.15 | 75.82 | -25.05 | 128.17 | 0.5139 | -894.0 | -777.9 | |
| 0.00 | 2.99 | 0.00 | 1.72 | -18.15 | 75.68 | -25.19 | 128.02 | 0.5155 | -770.0 | -646.3 | |
| 0.00 | 0.43 | 0.00 | 0.25 | -18.24 | 75.56 | -25.31 | 128.05 | 0.5177 | -698.0 | -672.4 | |
| 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. | |