| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.81 | 38.87 | 5.63 | 20.17 | -13.91 | 254.56 | -0.55 | 178.42 | 0.3021 | 466.5 | 283.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.27 | 0.00 | 0.66 | -12.33 | 259.86 | 4.76 | 196.68 | 0.2838 | 731.0 | 551.3 | |
| 0.00 | 0.64 | 0.00 | 0.33 | -13.54 | 259.38 | 4.28 | 194.01 | 0.3011 | 728.0 | 608.9 | |
| 0.00 | 1.18 | 0.00 | 0.61 | -13.25 | 259.35 | 4.24 | 194.14 | 0.2963 | 838.0 | 709.6 | |
| 0.00 | 1.73 | 0.00 | 0.89 | -12.84 | 259.18 | 4.08 | 193.96 | 0.2889 | 979.0 | 711.4 | |
| 0.00 | 1.00 | 0.00 | 0.52 | -14.17 | 258.10 | 3.00 | 189.56 | 0.3071 | 765.0 | 516.5 | |
| 0.00 | 1.54 | 0.00 | 0.80 | -13.72 | 258.07 | 2.96 | 189.69 | 0.2996 | 935.0 | 742.8 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -12.54 | 257.86 | 2.76 | 189.73 | 0.2796 | 571.0 | 548.0 | |
| 0.00 | 1.27 | 0.00 | 0.65 | -12.03 | 255.34 | 0.23 | 180.86 | 0.2670 | 903.0 | 679.8 | |
| 0.00 | 1.18 | 0.00 | 0.61 | -13.04 | 255.21 | 0.11 | 180.38 | 0.2840 | 902.0 | 642.4 | |
| 2.91 | 5.45 | 1.51 | 2.83 | -14.32 | 254.86 | -0.24 | 179.24 | 0.3054 | 1020.2 | 839.6 | |
| 0.00 | 1.00 | 0.00 | 0.51 | -11.93 | 254.87 | -0.23 | 179.14 | 0.2654 | 842.0 | 701.9 | |
| 4.36 | 6.54 | 2.27 | 3.40 | -14.42 | 254.61 | -0.49 | 178.45 | 0.3071 | 968.3 | 667.7 | |
| 1.00 | 2.00 | 0.52 | 1.04 | -14.61 | 253.57 | -1.53 | 175.22 | 0.3113 | 849.5 | 636.2 | |
| 0.00 | 0.82 | 0.00 | 0.43 | -15.93 | 252.29 | -2.81 | 171.89 | 0.3354 | -818.0 | -650.7 | |
| 2.54 | 4.36 | 1.33 | 2.28 | -15.25 | 251.57 | -3.53 | 169.48 | 0.3263 | -912.4 | -665.5 | |
| 0.00 | 1.54 | 0.00 | 0.81 | -14.61 | 251.59 | -3.52 | 169.12 | 0.3158 | -996.0 | -801.6 | |
| 0.00 | 3.45 | 0.00 | 1.80 | -14.96 | 251.55 | -3.55 | 169.23 | 0.3217 | -1062.0 | -851.5 | |
| 0.00 | 2.54 | 0.00 | 1.30 | -11.02 | 251.02 | -4.08 | 164.30 | 0.2594 | 873.0 | 727.9 | |
| 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. | |