| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.26 | 38.70 | 8.88 | 27.37 | -16.35 | 232.45 | -41.43 | 116.92 | 0.7118 | -113.8 | 51.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.00 | 0.00 | 0.64 | -17.20 | 239.83 | -34.05 | 122.43 | 0.6360 | 583.0 | 482.4 | |
| 1.36 | 3.27 | 0.90 | 2.15 | -14.17 | 236.34 | -37.54 | 115.96 | 0.6593 | 787.2 | 549.4 | |
| 0.00 | 1.27 | 0.00 | 0.89 | -20.06 | 234.81 | -39.07 | 122.94 | 0.7077 | 461.0 | 390.6 | |
| 0.00 | 1.00 | 0.00 | 0.66 | -14.24 | 235.97 | -37.91 | 115.87 | 0.6641 | 551.0 | 478.2 | |
| 0.64 | 1.82 | 0.42 | 1.20 | -14.37 | 235.86 | -38.02 | 115.99 | 0.6660 | 719.9 | 599.2 | |
| 0.00 | 3.54 | 0.00 | 2.37 | -14.74 | 235.34 | -38.54 | 116.22 | 0.6739 | 703.0 | 557.0 | |
| 0.00 | 3.63 | 0.00 | 2.44 | -15.26 | 235.19 | -38.69 | 116.85 | 0.6782 | 565.0 | 380.8 | |
| 0.00 | 1.00 | 0.00 | 0.67 | -14.97 | 235.17 | -38.71 | 116.44 | 0.6770 | 441.0 | 418.1 | |
| 0.45 | 1.54 | 0.31 | 1.05 | -14.40 | 234.24 | -39.64 | 115.17 | 0.6850 | 681.8 | 547.2 | |
| 0.00 | 1.18 | 0.00 | 0.81 | -15.28 | 233.92 | -39.96 | 116.19 | 0.6927 | -786.0 | -648.8 | |
| 0.00 | 1.27 | 0.00 | 0.88 | -14.91 | 233.42 | -40.46 | 115.44 | 0.6967 | -418.0 | -496.9 | |
| 0.00 | 1.73 | 0.00 | 1.21 | -16.31 | 232.96 | -40.92 | 117.06 | 0.7083 | -749.0 | -636.8 | |
| 0.00 | 0.55 | 0.00 | 0.38 | -15.97 | 232.62 | -41.26 | 116.45 | 0.7104 | -580.0 | -582.3 | |
| 0.00 | 1.18 | 0.00 | 0.84 | -16.02 | 231.97 | -41.91 | 116.20 | 0.7178 | -576.0 | -484.5 | |
| 6.09 | 13.90 | 4.50 | 10.28 | -17.46 | 229.99 | -43.89 | 117.09 | 0.7451 | -742.5 | -541.5 | |
| 3.72 | -15.00 | 2.75 | -15.00 | -17.14 | 229.96 | -43.92 | 116.67 | 0.7441 | -718.4 | 999999 | |
| 0.00 | 0.82 | 0.00 | 0.90 | -23.53 | 215.09 | -58.79 | 118.48 | 0.8940 | -106.0 | -122.3 | |
| 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. | |