| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.06 | 94.38 | 17.37 | 67.76 | 17.20 | 19.79 | 43.73 | 294.12 | 0.7252 | -405.9 | -256.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.72 | 0.00 | 1.39 | 21.10 | 24.92 | 48.86 | 297.08 | 0.7914 | -681.0 | -494.5 | |
| 6.42 | 33.84 | 4.74 | 24.93 | 16.92 | 21.50 | 45.44 | 293.05 | 0.7431 | -642.3 | -225.8 | |
| 4.16 | -2.00 | 3.05 | -2.00 | 17.01 | 21.08 | 45.02 | 293.32 | 0.7389 | -663.5 | 999999 | |
| 4.61 | 31.31 | 3.36 | 22.67 | 16.72 | 20.86 | 44.80 | 293.03 | 0.7355 | -760.6 | -506.2 | |
| 5.16 | -4.00 | 3.73 | -4.00 | 16.69 | 20.44 | 44.38 | 293.14 | 0.7309 | -894.4 | 999999 | |
| 0.00 | 1.00 | 0.00 | 0.74 | 19.58 | 21.11 | 45.05 | 296.62 | 0.7482 | -167.0 | -238.5 | |
| 0.00 | 0.81 | 0.00 | 0.59 | 17.46 | 19.87 | 43.81 | 294.36 | 0.7273 | -494.0 | -429.0 | |
| 0.00 | 1.72 | 0.00 | 1.19 | 16.50 | 17.60 | 41.54 | 294.00 | 0.6983 | -383.0 | -384.2 | |
| 0.00 | 1.63 | 0.00 | 1.13 | 17.23 | 17.72 | 41.66 | 294.95 | 0.7024 | -577.0 | -499.5 | |
| 0.00 | 1.18 | 0.00 | 0.82 | 17.43 | 17.64 | 41.58 | 295.24 | 0.7023 | -496.0 | -478.1 | |
| 0.36 | 1.90 | 0.25 | 1.31 | 16.95 | 17.47 | 41.41 | 294.66 | 0.6985 | -826.8 | -712.1 | |
| 0.00 | 2.71 | 0.00 | 1.87 | 17.04 | 17.24 | 41.18 | 294.89 | 0.6963 | -771.0 | -650.8 | |
| 0.00 | 1.36 | 0.00 | 0.93 | 17.11 | 16.92 | 40.86 | 295.12 | 0.6928 | -742.0 | -661.5 | |
| 0.00 | 0.90 | 0.00 | 0.62 | 20.45 | 16.03 | 39.97 | 300.07 | 0.6977 | 380.0 | 288.3 | |
| 0.00 | 1.45 | 0.00 | 0.96 | 16.63 | 14.89 | 38.82 | 295.39 | 0.6672 | 715.0 | 620.5 | |
| 3.35 | 8.32 | 2.24 | 5.58 | 17.97 | 15.02 | 38.96 | 297.21 | 0.6748 | 731.9 | 475.1 | |
| 0.00 | 3.17 | 0.00 | 2.13 | 19.00 | 15.09 | 39.03 | 298.59 | 0.6804 | 778.0 | 575.8 | |
| 0.00 | 1.36 | 0.00 | 0.90 | 19.35 | 13.87 | 37.81 | 299.73 | 0.6684 | 466.0 | 419.4 | |
| 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. | |