| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 70.95 | 432.47 | 37.14 | 226.46 | 12.55 | 13.56 | -0.02 | 0.09 | 0.3237 | -1086.1 | -389.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 70.69 | 406.70 | 37.00 | 212.99 | 12.58 | 13.71 | 0.13 | 359.61 | 0.3240 | -1547.8 | -438.4 | |
| 0.26 | -1.00 | 0.14 | -1.00 | 13.22 | 13.40 | -0.18 | 0.52 | 0.3345 | -815.3 | 999999 | |
| 0.00 | 1.76 | 0.00 | 0.91 | 9.48 | 12.64 | -0.94 | 3.42 | 0.2724 | 894.0 | 727.5 | |
| 0.00 | 1.58 | 0.00 | 0.83 | 12.94 | 12.45 | -1.13 | 3.36 | 0.3304 | -687.0 | -522.4 | |
| 0.00 | 1.32 | 0.00 | 0.69 | 11.26 | 11.96 | -1.62 | 5.26 | 0.3032 | -826.0 | -645.7 | |
| 0.00 | 1.23 | 0.00 | 0.64 | 11.89 | 11.87 | -1.71 | 5.37 | 0.3138 | -667.0 | -553.4 | |
| 0.00 | 1.50 | 0.00 | 0.78 | 11.74 | 11.84 | -1.74 | 5.51 | 0.3113 | -878.0 | -760.0 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 12.15 | 11.83 | -1.74 | 5.39 | 0.3181 | -649.0 | -487.9 | |
| 0.00 | 1.23 | 0.00 | 0.64 | 12.05 | 11.71 | -1.87 | 5.80 | 0.3167 | -604.0 | -427.7 | |
| 0.00 | 2.29 | 0.00 | 1.20 | 12.31 | 11.43 | -2.14 | 6.56 | 0.3214 | -666.0 | -332.6 | |
| 0.00 | 2.46 | 0.00 | 1.28 | 11.27 | 11.04 | -2.54 | 8.21 | 0.3051 | 1011.0 | 714.0 | |
| 0.00 | 1.32 | 0.00 | 0.69 | 10.98 | 11.01 | -2.56 | 8.44 | 0.3005 | 762.0 | 639.7 | |
| 0.00 | 1.58 | 0.00 | 0.82 | 11.43 | 10.77 | -2.81 | 9.01 | 0.3084 | 865.0 | 647.2 | |
| 0.00 | 5.37 | 0.00 | 2.82 | 12.72 | 10.72 | -2.86 | 8.51 | 0.3298 | 1103.0 | 887.6 | |
| 0.00 | 1.85 | 0.00 | 0.97 | 11.93 | 10.58 | -3.00 | 9.33 | 0.3172 | 1060.0 | 825.5 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 11.13 | 9.05 | -4.53 | 14.56 | 0.3093 | 852.0 | 635.8 | |
| 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. | |