| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 77.97 | 484.73 | 44.06 | 274.21 | -16.43 | 13.59 | -26.65 | 116.91 | 0.4843 | 997.1 | 368.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.02 | 0.00 | 0.58 | -20.79 | 15.90 | -24.34 | 127.02 | 0.4846 | 716.0 | 572.2 | |
| 0.00 | 1.79 | 0.00 | 0.99 | -16.17 | 16.47 | -23.78 | 118.73 | 0.4435 | -892.0 | -730.4 | |
| 44.38 | 474.43 | 24.97 | 268.18 | -16.47 | 14.22 | -26.02 | 117.44 | 0.4760 | 1385.9 | 388.5 | |
| 2.64 | -3.00 | 1.49 | -3.00 | -16.94 | 13.98 | -26.26 | 118.17 | 0.4822 | 695.5 | 999999 | |
| 0.68 | -3.00 | 0.39 | -3.00 | -16.41 | 13.44 | -26.80 | 116.74 | 0.4864 | 1053.6 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -17.65 | 13.24 | -27.00 | 118.92 | 0.4963 | 377.0 | 234.8 | |
| 6.63 | -3.00 | 3.76 | -3.00 | -16.55 | 13.18 | -27.07 | 116.82 | 0.4908 | 1198.0 | 999999 | |
| 23.64 | -3.00 | 13.45 | -3.00 | -16.24 | 12.77 | -27.47 | 115.93 | 0.4945 | 1222.1 | 999999 | |
| 0.00 | 1.62 | 0.00 | 0.96 | -16.82 | 8.20 | -32.04 | 114.19 | 0.5589 | -832.0 | -618.3 | |
| 0.00 | 0.77 | 0.00 | 0.46 | -16.35 | 7.74 | -32.50 | 113.15 | 0.5629 | -575.0 | -541.9 | |
| 0.00 | 0.51 | 0.00 | 0.31 | -14.78 | 7.08 | -33.16 | 110.16 | 0.5656 | -706.0 | -550.5 | |
| 0.00 | 1.19 | 0.00 | 0.72 | -16.28 | 6.69 | -33.55 | 112.52 | 0.5765 | -641.0 | -554.8 | |
| 0.00 | 1.02 | 0.00 | 0.62 | -16.19 | 6.04 | -34.20 | 112.07 | 0.5847 | -703.0 | -538.8 | |
| 0.00 | 1.02 | 0.00 | 0.62 | -15.27 | 5.74 | -34.50 | 110.42 | 0.5853 | -888.0 | -660.3 | |
| 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. | |