| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.67 | 376.97 | 44.58 | 259.49 | 23.17 | 156.06 | -42.33 | 63.15 | 0.6960 | -867.2 | -293.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.32 | 0.00 | 0.91 | 26.47 | 156.58 | -41.81 | 58.44 | 0.7027 | -820.0 | -724.7 | |
| 0.00 | 0.97 | 0.00 | 0.67 | 26.44 | 156.27 | -42.11 | 58.60 | 0.7058 | -501.0 | -472.3 | |
| 14.85 | 295.60 | 10.09 | 201.78 | 22.64 | 156.77 | -41.62 | 63.64 | 0.6864 | -1148.5 | -348.8 | |
| 27.15 | -3.00 | 18.58 | -3.00 | 23.12 | 156.37 | -42.02 | 63.12 | 0.6925 | -1091.1 | 999999 | |
| 1.67 | -3.00 | 1.14 | -3.00 | 22.24 | 156.44 | -41.95 | 64.33 | 0.6888 | -829.0 | 999999 | |
| 0.35 | -3.00 | 0.24 | -3.00 | 22.47 | 156.17 | -42.21 | 64.09 | 0.6925 | -440.0 | 999999 | |
| 16.87 | 70.12 | 11.84 | 49.41 | 24.10 | 154.99 | -43.39 | 62.25 | 0.7110 | -904.5 | -130.1 | |
| 1.93 | -7.00 | 1.36 | -7.00 | 23.76 | 154.68 | -43.70 | 62.82 | 0.7132 | -582.0 | 999999 | |
| 0.88 | 1.93 | 0.60 | 1.32 | 19.89 | 155.56 | -42.82 | 67.93 | 0.6920 | 477.3 | 419.8 | |
| 0.97 | 2.99 | 0.73 | 2.27 | 24.77 | 150.41 | -47.97 | 62.79 | 0.7607 | 682.9 | 474.9 | |
| 0.00 | 0.79 | 0.00 | 0.59 | 22.64 | 150.52 | -47.86 | 65.52 | 0.7543 | 561.0 | 537.7 | |
| 0.00 | 2.11 | 0.00 | 1.67 | 26.20 | 148.61 | -49.77 | 61.46 | 0.7820 | 592.0 | 490.9 | |
| 0.00 | 1.14 | 0.00 | 0.87 | 23.22 | 149.90 | -48.48 | 64.91 | 0.7620 | 372.0 | 370.9 | |
| 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. | |