| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.79 | 0.00 | 9.59 | -5.31 | 139.03 | -19.85 | 120.67 | 0.3949 | -851.6 | -716.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.88 | 0.00 | 0.47 | -4.23 | 140.96 | -17.93 | 120.82 | 0.3590 | -825.0 | -697.7 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -4.31 | 140.64 | -18.25 | 120.54 | 0.3641 | -797.0 | -631.5 | |
| 0.00 | 1.41 | 0.00 | 0.75 | -4.66 | 140.09 | -18.80 | 120.60 | 0.3747 | -934.0 | -813.1 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -4.16 | 139.72 | -19.16 | 118.94 | 0.3758 | -933.0 | -718.6 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -5.26 | 139.56 | -19.33 | 121.24 | 0.3871 | -767.0 | -611.2 | |
| 0.00 | 2.11 | 0.00 | 1.14 | -5.73 | 139.51 | -19.37 | 122.19 | 0.3917 | -1009.0 | -871.6 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -4.16 | 139.56 | -19.32 | 118.75 | 0.3781 | -958.0 | -864.8 | |
| 0.00 | 2.11 | 0.00 | 1.14 | -5.54 | 139.45 | -19.43 | 121.71 | 0.3909 | -939.0 | -706.5 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -3.89 | 139.47 | -19.41 | 118.00 | 0.3772 | -1082.0 | -887.2 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -6.29 | 139.17 | -19.72 | 122.93 | 0.4012 | -826.0 | -747.2 | |
| 0.00 | 1.76 | 0.00 | 0.96 | -7.44 | 138.18 | -20.70 | 123.95 | 0.4244 | -740.0 | -602.7 | |
| 0.00 | 1.41 | 0.00 | 0.77 | -6.45 | 138.20 | -20.69 | 121.99 | 0.4157 | -728.0 | -602.4 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -4.25 | 135.91 | -22.97 | 114.81 | 0.4306 | -651.0 | -587.0 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -5.09 | 135.75 | -23.13 | 116.38 | 0.4387 | -733.0 | -632.8 | |
| 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. | |