| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.19 | 132.08 | 26.06 | 72.86 | -16.70 | 242.46 | -12.43 | 152.05 | 0.4403 | -238.9 | -222.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.81 | 6.69 | 0.97 | 3.60 | -15.07 | 245.94 | -8.96 | 157.41 | 0.3929 | 979.0 | 951.2 | |
| 1.63 | -1.00 | 0.88 | -1.00 | -14.88 | 245.78 | -9.11 | 156.87 | 0.3910 | 1132.2 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -15.50 | 245.69 | -9.20 | 157.29 | 0.4007 | 760.0 | 582.6 | |
| 0.00 | 1.81 | 0.00 | 0.98 | -15.61 | 245.24 | -9.65 | 156.41 | 0.4052 | 713.0 | 565.8 | |
| 0.00 | 1.18 | 0.00 | 0.64 | -16.61 | 244.38 | -10.51 | 155.63 | 0.4252 | -1061.0 | -861.1 | |
| 2.53 | 68.61 | 1.39 | 37.68 | -16.72 | 243.96 | -10.93 | 154.87 | 0.4295 | -1189.0 | -166.9 | |
| 0.72 | -6.00 | 0.40 | -6.00 | -16.35 | 243.91 | -10.98 | 154.41 | 0.4247 | -1012.4 | 999999 | |
| 1.45 | -6.00 | 0.79 | -6.00 | -16.76 | 243.66 | -11.23 | 154.33 | 0.4321 | -547.9 | 999999 | |
| 4.52 | -6.00 | 2.49 | -6.00 | -16.99 | 243.52 | -11.37 | 154.29 | 0.4364 | -1027.3 | 999999 | |
| 0.54 | 1.36 | 0.29 | 0.74 | -15.34 | 243.62 | -11.27 | 152.68 | 0.4125 | 532.8 | 827.2 | |
| 10.49 | -6.00 | 5.75 | -6.00 | -16.63 | 243.48 | -11.41 | 153.82 | 0.4315 | 931.3 | 999999 | |
| 3.71 | -6.00 | 2.04 | -6.00 | -16.57 | 243.03 | -11.86 | 152.87 | 0.4339 | 816.3 | 999999 | |
| 0.00 | 2.44 | 0.00 | 1.33 | -15.78 | 242.95 | -11.94 | 151.83 | 0.4236 | 882.0 | 671.4 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -16.45 | 242.55 | -12.34 | 151.81 | 0.4358 | -73.0 | -120.2 | |
| 0.72 | 6.78 | 0.40 | 3.77 | -16.66 | 240.71 | -14.18 | 148.64 | 0.4529 | -897.2 | -866.1 | |
| 0.00 | 2.17 | 0.00 | 1.21 | -17.10 | 240.58 | -14.31 | 148.92 | 0.4597 | -910.0 | -704.2 | |
| 19.07 | 38.87 | 10.66 | 21.72 | -17.18 | 240.14 | -14.75 | 148.26 | 0.4642 | -1034.1 | -507.7 | |
| 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. | |