| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.66 | 0.00 | 11.17 | -19.45 | 164.82 | -17.32 | 131.85 | 0.3932 | -705.4 | -608.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.80 | 0.00 | 0.45 | -32.64 | 190.18 | 8.04 | 194.30 | 0.4790 | 670.0 | 558.7 | |
| 0.00 | 2.13 | 0.00 | 1.10 | -17.46 | 170.73 | -11.41 | 138.68 | 0.2872 | -763.0 | -719.6 | |
| 0.00 | 1.51 | 0.00 | 0.78 | -14.39 | 169.38 | -12.76 | 127.25 | 0.2700 | -679.0 | -406.5 | |
| 0.00 | 1.33 | 0.00 | 0.72 | -24.52 | 167.98 | -14.16 | 146.32 | 0.4031 | -718.0 | -561.5 | |
| 0.00 | 2.48 | 0.00 | 1.30 | -18.30 | 168.00 | -14.14 | 134.75 | 0.3280 | -911.0 | -722.8 | |
| 0.00 | 0.98 | 0.00 | 0.53 | -20.15 | 163.99 | -18.15 | 131.97 | 0.3950 | -838.0 | -703.9 | |
| 0.00 | 1.33 | 0.00 | 0.71 | -16.78 | 162.17 | -19.97 | 122.30 | 0.3885 | -880.0 | -743.2 | |
| 0.00 | 1.77 | 0.00 | 0.98 | -22.24 | 161.41 | -20.74 | 132.40 | 0.4456 | -934.0 | -775.7 | |
| 0.00 | 2.04 | 0.00 | 1.13 | -21.80 | 161.30 | -20.84 | 131.46 | 0.4426 | -713.0 | -619.4 | |
| 0.00 | 0.44 | 0.00 | 0.24 | -12.53 | 162.08 | -20.06 | 111.76 | 0.3621 | -678.0 | -489.6 | |
| 0.00 | 0.80 | 0.00 | 0.42 | -10.04 | 161.94 | -20.20 | 104.91 | 0.3534 | -895.0 | -670.2 | |
| 0.00 | 1.42 | 0.00 | 0.78 | -18.45 | 160.34 | -21.80 | 123.83 | 0.4259 | -900.0 | -734.9 | |
| 0.00 | 1.15 | 0.00 | 0.62 | -11.48 | 159.76 | -22.38 | 107.38 | 0.3927 | -838.0 | -675.2 | |
| 0.00 | 2.48 | 0.00 | 1.41 | -23.39 | 157.91 | -24.23 | 130.37 | 0.4964 | -799.0 | -596.1 | |
| 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. | |