| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.39 | 25.65 | 3.61 | 14.36 | -17.62 | 100.25 | 16.63 | 216.16 | 0.4666 | -74.2 | -59.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.12 | 0.00 | 0.65 | -19.51 | 105.36 | 21.75 | 221.53 | 0.5288 | 165.0 | 302.5 | |
| 0.60 | 3.46 | 0.34 | 1.94 | -14.95 | 104.15 | 20.53 | 226.60 | 0.4684 | -891.6 | -737.6 | |
| 3.89 | 10.71 | 2.20 | 6.07 | -16.81 | 104.11 | 20.50 | 223.67 | 0.4875 | 826.7 | 732.1 | |
| 1.90 | -3.00 | 1.07 | -3.00 | -16.62 | 104.03 | 20.41 | 223.84 | 0.4845 | 1009.0 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -16.76 | 100.86 | 17.24 | 218.92 | 0.4538 | 761.0 | 645.4 | |
| 0.00 | 1.30 | 0.00 | 0.72 | -17.74 | 100.30 | 16.68 | 216.64 | 0.4601 | 585.0 | 396.0 | |
| 0.00 | 0.60 | 0.00 | 0.33 | -17.69 | 98.16 | 14.54 | 213.05 | 0.4404 | 535.0 | 425.4 | |
| 0.00 | 0.69 | 0.00 | 0.38 | -17.51 | 95.04 | 11.42 | 207.33 | 0.4131 | -730.0 | -607.6 | |
| 0.00 | 0.95 | 0.00 | 0.52 | -18.00 | 93.76 | 10.15 | 204.15 | 0.4113 | -808.0 | -645.6 | |
| 0.00 | 1.64 | 0.00 | 0.89 | -18.19 | 93.68 | 10.07 | 203.78 | 0.4135 | -688.0 | -476.5 | |
| 0.00 | 0.69 | 0.00 | 0.37 | -17.84 | 93.60 | 9.98 | 203.97 | 0.4079 | -883.0 | -754.6 | |
| 0.00 | 1.04 | 0.00 | 0.57 | -21.05 | 90.96 | 7.34 | 195.75 | 0.4413 | -473.0 | -494.1 | |
| 0.00 | 1.12 | 0.00 | 0.62 | -21.66 | 89.96 | 6.34 | 193.35 | 0.4467 | -658.0 | -583.5 | |
| 0.00 | 1.47 | 0.00 | 0.82 | -22.99 | 89.89 | 6.27 | 192.50 | 0.4665 | -668.0 | -642.2 | |
| 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. | |