| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.28 | 28.31 | 7.33 | 19.50 | 13.33 | 91.32 | -43.94 | 77.55 | 0.6916 | 309.9 | 171.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.05 | 0.00 | 0.60 | 11.97 | 105.85 | -29.41 | 77.21 | 0.4945 | 836.0 | 635.8 | |
| 0.00 | 0.97 | 0.00 | 0.56 | 13.00 | 104.66 | -30.60 | 75.55 | 0.5143 | 710.0 | 580.2 | |
| 0.00 | 1.85 | 0.00 | 1.13 | 12.46 | 99.28 | -35.98 | 77.77 | 0.5891 | -780.0 | -608.7 | |
| 0.00 | 0.62 | 0.00 | 0.39 | 14.45 | 97.22 | -38.04 | 74.90 | 0.6203 | -675.0 | -497.9 | |
| 0.00 | 0.44 | 0.00 | 0.28 | 7.96 | 97.02 | -38.24 | 85.43 | 0.6172 | -620.0 | -652.8 | |
| 0.00 | 1.76 | 0.00 | 1.11 | 7.84 | 96.91 | -38.34 | 85.64 | 0.6187 | -569.0 | -457.8 | |
| 0.00 | 0.88 | 0.00 | 0.56 | 11.07 | 95.74 | -39.52 | 80.50 | 0.6355 | -516.0 | -424.7 | |
| 0.00 | 0.79 | 0.00 | 0.54 | 17.08 | 92.40 | -42.86 | 71.95 | 0.6862 | 181.0 | 174.9 | |
| 0.00 | 0.44 | 0.00 | 0.31 | 14.25 | 90.26 | -45.00 | 76.35 | 0.7076 | -611.0 | -509.2 | |
| 0.00 | 1.05 | 0.00 | 0.76 | 16.59 | 88.84 | -46.42 | 73.30 | 0.7272 | 520.0 | 417.9 | |
| 10.28 | 13.71 | 7.33 | 9.77 | 13.27 | 89.04 | -46.22 | 77.85 | 0.7211 | 850.9 | 551.3 | |
| 0.00 | 0.53 | 0.00 | 0.37 | 12.10 | 89.27 | -45.99 | 79.46 | 0.7177 | 489.0 | 408.7 | |
| 0.00 | 0.88 | 0.00 | 0.63 | 13.56 | 88.56 | -46.70 | 77.49 | 0.7270 | 459.0 | 370.9 | |
| 0.00 | 2.55 | 0.00 | 1.88 | 14.91 | 87.13 | -48.13 | 75.79 | 0.7445 | 444.0 | 494.1 | |
| 0.00 | 0.79 | 0.00 | 0.61 | 19.08 | 85.63 | -49.63 | 70.50 | 0.7662 | 505.0 | 439.9 | |
| 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. | |