| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.59 | 219.57 | 21.70 | 137.63 | 5.89 | 45.20 | 36.24 | 285.67 | 0.6126 | -804.2 | -367.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.70 | 0.00 | 1.36 | 10.52 | 58.68 | 49.71 | 287.17 | 0.7873 | -491.0 | -420.6 | |
| 0.00 | 1.36 | 0.00 | 1.09 | 10.81 | 58.56 | 49.59 | 287.58 | 0.7869 | -678.0 | -566.8 | |
| 34.59 | 202.68 | 21.70 | 127.21 | 5.85 | 45.43 | 36.47 | 285.53 | 0.6160 | -1126.5 | -385.9 | |
| 0.00 | 0.59 | 0.00 | 0.36 | 7.23 | 42.14 | 33.17 | 289.35 | 0.5776 | -694.0 | -621.9 | |
| 0.00 | 1.10 | 0.00 | 0.67 | 8.26 | 42.06 | 33.09 | 291.07 | 0.5812 | -573.0 | -388.7 | |
| 0.00 | 1.10 | 0.00 | 0.67 | 7.50 | 41.95 | 32.98 | 289.89 | 0.5762 | -664.0 | -565.2 | |
| 0.00 | 1.02 | 0.00 | 0.62 | 7.64 | 41.71 | 32.75 | 290.25 | 0.5737 | -628.0 | -574.1 | |
| 0.00 | 1.19 | 0.00 | 0.68 | -2.62 | 38.82 | 29.85 | 272.58 | 0.4998 | 716.0 | 600.0 | |
| 0.00 | 1.70 | 0.00 | 0.96 | 0.65 | 37.67 | 28.71 | 279.46 | 0.4889 | 580.0 | 572.2 | |
| 0.00 | 1.36 | 0.00 | 0.78 | 7.19 | 36.45 | 27.48 | 292.94 | 0.4992 | -815.0 | -692.2 | |
| 0.00 | 1.44 | 0.00 | 0.82 | 7.57 | 36.20 | 27.24 | 293.84 | 0.4980 | -935.0 | -783.7 | |
| 0.00 | 1.02 | 0.00 | 0.58 | 7.33 | 36.09 | 27.12 | 293.47 | 0.4950 | -728.0 | -564.6 | |
| 0.00 | 1.53 | 0.00 | 0.89 | 11.86 | 36.19 | 27.22 | 301.38 | 0.5265 | 720.0 | 581.2 | |
| 0.00 | 1.78 | 0.00 | 0.94 | -3.47 | 28.80 | 19.83 | 272.25 | 0.3404 | 729.0 | 588.5 | |
| 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. | |