| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.56 | 43.45 | 12.35 | 34.68 | -23.51 | 94.95 | -46.57 | 121.85 | 0.7860 | 8.8 | 77.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.70 | 6.33 | 3.63 | 4.89 | -23.25 | 96.60 | -44.92 | 122.27 | 0.7696 | 679.4 | 424.2 | |
| 3.08 | 11.97 | 2.41 | 9.39 | -24.08 | 96.14 | -45.37 | 123.04 | 0.7774 | 808.4 | 510.1 | |
| 0.00 | 0.60 | 0.00 | 0.47 | -24.47 | 95.87 | -45.65 | 123.38 | 0.7817 | -174.0 | -121.1 | |
| 0.00 | 2.14 | 0.00 | 1.68 | -23.82 | 95.98 | -45.53 | 122.66 | 0.7778 | 704.0 | 494.2 | |
| 0.94 | 2.22 | 0.74 | 1.74 | -23.62 | 95.93 | -45.58 | 122.40 | 0.7774 | 596.7 | 437.7 | |
| 0.00 | 0.77 | 0.00 | 0.62 | -23.81 | 94.63 | -46.89 | 122.04 | 0.7902 | 320.0 | 232.3 | |
| 0.00 | 1.11 | 0.00 | 0.89 | -23.25 | 94.79 | -46.72 | 121.45 | 0.7864 | 364.0 | 269.4 | |
| 4.96 | 7.36 | 4.01 | 5.95 | -23.23 | 94.09 | -47.43 | 121.13 | 0.7928 | -723.6 | -510.2 | |
| 0.00 | 0.86 | 0.00 | 0.70 | -23.21 | 93.52 | -47.99 | 120.86 | 0.7979 | -395.0 | -380.8 | |
| 0.00 | 2.05 | 0.00 | 1.69 | -23.18 | 93.30 | -48.22 | 120.74 | 0.7998 | -599.0 | -480.0 | |
| 0.00 | 0.77 | 0.00 | 0.64 | -23.58 | 92.86 | -48.66 | 121.02 | 0.8053 | -363.0 | -358.6 | |
| 0.00 | 1.97 | 0.00 | 1.62 | -22.73 | 93.12 | -48.39 | 120.14 | 0.7997 | -600.0 | -412.8 | |
| 0.00 | 0.94 | 0.00 | 0.78 | -23.42 | 92.74 | -48.78 | 120.79 | 0.8057 | -238.0 | -221.5 | |
| 1.88 | 4.36 | 1.56 | 3.62 | -23.13 | 92.74 | -48.78 | 120.45 | 0.8047 | -503.0 | -403.9 | |
| 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. | |