| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66.43 | 207.91 | 37.00 | 115.80 | -16.69 | 194.84 | 23.37 | 236.40 | 0.4577 | 118.4 | 48.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.81 | 0.00 | 0.46 | -15.69 | 198.89 | 27.42 | 241.93 | 0.5045 | 811.0 | 625.9 | |
| 2.16 | 81.44 | 1.22 | 46.10 | -17.95 | 196.61 | 25.14 | 235.87 | 0.4902 | 678.0 | 399.7 | |
| 0.00 | 4.13 | 0.00 | 2.33 | -17.04 | 196.44 | 24.97 | 237.35 | 0.4813 | 788.0 | 657.2 | |
| 0.00 | 1.89 | 0.00 | 1.07 | -18.36 | 196.53 | 25.06 | 235.06 | 0.4924 | 285.0 | 304.3 | |
| 24.36 | -2.00 | 13.78 | -2.00 | -17.67 | 196.39 | 24.92 | 236.16 | 0.4854 | 1083.5 | 999999 | |
| 8.18 | 13.12 | 4.60 | 7.37 | -16.76 | 196.02 | 24.55 | 237.46 | 0.4738 | 1034.3 | 793.5 | |
| 0.00 | 1.44 | 0.00 | 0.81 | -17.27 | 195.81 | 24.34 | 236.32 | 0.4749 | 378.0 | 293.6 | |
| 0.00 | 1.17 | 0.00 | 0.65 | -15.31 | 195.10 | 23.64 | 239.38 | 0.4512 | 692.0 | 556.2 | |
| 0.72 | 6.02 | 0.40 | 3.36 | -16.75 | 194.97 | 23.51 | 236.45 | 0.4602 | 1043.4 | 779.3 | |
| 0.00 | 2.79 | 0.00 | 1.53 | -15.51 | 193.80 | 22.33 | 237.63 | 0.4352 | -681.0 | -555.7 | |
| 4.04 | 95.10 | 2.22 | 52.12 | -15.49 | 193.28 | 21.81 | 237.12 | 0.4282 | -1100.0 | -427.5 | |
| 11.42 | -11.00 | 6.27 | -11.00 | -16.18 | 193.19 | 21.72 | 235.62 | 0.4325 | -1004.3 | 999999 | |
| 6.83 | -11.00 | 3.74 | -11.00 | -15.86 | 193.12 | 21.65 | 236.17 | 0.4291 | -1157.9 | 999999 | |
| 8.72 | -11.00 | 4.77 | -11.00 | -15.37 | 193.03 | 21.56 | 237.09 | 0.4239 | -1251.5 | 999999 | |
| 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. | |