| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.05 | 0.00 | 11.49 | 9.73 | 185.49 | 4.88 | 279.74 | 0.1062 | -777.7 | -695.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.34 | 0.00 | 0.67 | 5.93 | 187.73 | 7.11 | 259.92 | 0.1257 | -831.0 | -696.2 | |
| 0.00 | 1.25 | 0.00 | 0.62 | 6.03 | 187.27 | 6.66 | 260.01 | 0.1176 | -944.0 | -735.8 | |
| 0.00 | 2.50 | 0.00 | 1.25 | 12.21 | 186.37 | 5.76 | 311.70 | 0.1319 | -846.0 | -712.4 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 11.46 | 186.26 | 5.65 | 307.56 | 0.1222 | -986.0 | -805.8 | |
| 0.00 | 2.15 | 0.00 | 1.07 | 11.37 | 185.95 | 5.33 | 308.53 | 0.1170 | -868.0 | -829.7 | |
| 0.00 | 2.77 | 0.00 | 1.38 | 10.92 | 185.82 | 5.20 | 305.99 | 0.1105 | -1034.0 | -916.0 | |
| 0.00 | 1.61 | 0.00 | 0.80 | 5.72 | 185.62 | 5.00 | 253.28 | 0.0910 | -965.0 | -787.2 | |
| 0.00 | 1.34 | 0.00 | 0.67 | 10.71 | 185.60 | 4.98 | 305.55 | 0.1053 | -927.0 | -822.3 | |
| 0.00 | 0.89 | 0.00 | 0.45 | 11.28 | 185.55 | 4.93 | 310.11 | 0.1107 | -901.0 | -734.3 | |
| 0.00 | 0.72 | 0.00 | 0.36 | 5.90 | 185.32 | 4.70 | 254.31 | 0.0851 | -867.0 | -759.4 | |
| 0.00 | 4.02 | 0.00 | 2.00 | 11.04 | 185.36 | 4.74 | 309.46 | 0.1055 | -808.0 | -751.0 | |
| 0.00 | 1.25 | 0.00 | 0.62 | 6.12 | 185.14 | 4.52 | 256.23 | 0.0811 | -967.0 | -759.4 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 10.02 | 184.39 | 3.77 | 307.04 | 0.0815 | -867.0 | -670.5 | |
| 0.00 | 1.25 | 0.00 | 0.62 | 10.07 | 178.86 | -1.76 | 31.40 | 0.0583 | 923.0 | 724.9 | |
| 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. | |