| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.28 | 40.13 | 3.87 | 21.68 | -19.81 | 141.27 | -18.32 | 131.85 | 0.3951 | 288.4 | 172.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.53 | 8.43 | 2.36 | 4.39 | -17.57 | 146.66 | -12.92 | 135.90 | 0.3078 | 1110.4 | 767.3 | |
| 0.00 | 1.24 | 0.00 | 0.65 | -17.26 | 146.53 | -13.06 | 134.86 | 0.3058 | 859.0 | 721.1 | |
| 0.00 | 2.49 | 0.00 | 1.32 | -19.07 | 144.21 | -15.38 | 134.51 | 0.3529 | 877.0 | 678.5 | |
| 0.00 | 2.04 | 0.00 | 1.08 | -18.64 | 144.22 | -15.37 | 133.58 | 0.3481 | 1030.0 | 847.0 | |
| 0.00 | 0.80 | 0.00 | 0.42 | -17.10 | 143.31 | -16.28 | 128.51 | 0.3438 | 856.0 | 690.9 | |
| 0.00 | 1.15 | 0.00 | 0.63 | -21.86 | 141.61 | -17.98 | 135.76 | 0.4123 | 706.0 | 572.1 | |
| 1.15 | 3.11 | 0.62 | 1.67 | -20.13 | 141.56 | -18.03 | 132.38 | 0.3951 | 1021.1 | 861.3 | |
| 0.00 | 2.22 | 0.00 | 1.21 | -21.89 | 140.75 | -18.84 | 134.58 | 0.4224 | 830.0 | 576.6 | |
| 0.00 | 1.60 | 0.00 | 0.87 | -20.75 | 140.19 | -19.40 | 131.65 | 0.4174 | 784.0 | 654.0 | |
| 0.00 | 2.22 | 0.00 | 1.21 | -19.51 | 139.67 | -19.92 | 128.53 | 0.4122 | 892.0 | 648.2 | |
| 0.00 | 1.95 | 0.00 | 1.06 | -19.76 | 139.54 | -20.05 | 128.85 | 0.4161 | 291.0 | 352.2 | |
| 0.00 | 0.71 | 0.00 | 0.39 | -20.52 | 138.05 | -21.53 | 128.51 | 0.4412 | -790.0 | -620.8 | |
| 1.33 | 7.90 | 0.74 | 4.40 | -21.54 | 137.44 | -22.15 | 129.68 | 0.4575 | -1065.3 | -800.3 | |
| 0.27 | -13.00 | 0.15 | -13.00 | -21.44 | 137.35 | -22.24 | 129.41 | 0.4577 | -1023.0 | 999999 | |
| 0.00 | 0.98 | 0.00 | 0.54 | -20.37 | 137.28 | -22.31 | 127.34 | 0.4494 | -778.0 | -645.8 | |
| 0.00 | 1.60 | 0.00 | 0.89 | -20.78 | 136.30 | -23.28 | 127.03 | 0.4649 | -835.0 | -693.1 | |
| 0.00 | 1.69 | 0.00 | 0.95 | -21.19 | 135.49 | -24.09 | 126.94 | 0.4782 | -857.0 | -767.7 | |
| 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. | |