| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.72 | 371.90 | 33.59 | 196.20 | -1.40 | 154.79 | 18.43 | 247.23 | 0.3441 | 1136.5 | 431.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 51.50 | 313.46 | 27.20 | 165.67 | -1.40 | 155.09 | 18.73 | 247.62 | 0.3486 | 1477.2 | 417.4 | |
| 2.64 | 29.70 | 1.39 | 15.59 | -1.90 | 153.96 | 17.59 | 244.90 | 0.3351 | 969.9 | 612.2 | |
| 0.26 | -2.00 | 0.14 | -2.00 | -2.02 | 153.92 | 17.56 | 244.53 | 0.3355 | 849.0 | 999999 | |
| 1.76 | -2.00 | 0.92 | -2.00 | -1.69 | 153.83 | 17.47 | 245.32 | 0.3316 | 1223.8 | 999999 | |
| 0.00 | 1.85 | 0.00 | 0.97 | -0.50 | 153.73 | 17.37 | 248.52 | 0.3222 | 1033.0 | 814.2 | |
| 0.00 | 6.15 | 0.00 | 3.22 | -1.10 | 153.64 | 17.27 | 246.69 | 0.3247 | 966.0 | 913.4 | |
| 1.14 | -2.00 | 0.60 | -2.00 | -1.62 | 153.58 | 17.21 | 245.18 | 0.3274 | 992.5 | 999999 | |
| 6.42 | 12.22 | 3.34 | 6.36 | -0.27 | 153.10 | 16.74 | 248.44 | 0.3110 | 1122.4 | 764.6 | |
| 0.00 | 1.32 | 0.00 | 0.69 | -3.33 | 153.09 | 16.73 | 239.90 | 0.3337 | 797.0 | 604.5 | |
| 0.00 | 1.23 | 0.00 | 0.64 | 0.25 | 152.04 | 15.68 | 248.69 | 0.2913 | 808.0 | 671.4 | |
| 0.00 | 1.05 | 0.00 | 0.54 | -1.72 | 150.12 | 13.76 | 239.44 | 0.2773 | -633.0 | -466.5 | |
| 0.00 | 1.14 | 0.00 | 0.59 | -2.32 | 150.00 | 13.64 | 237.37 | 0.2810 | -997.0 | -855.2 | |
| 0.00 | 1.58 | 0.00 | 0.81 | -1.89 | 149.69 | 13.33 | 238.08 | 0.2727 | -931.0 | -821.3 | |
| 0.00 | 2.20 | 0.00 | 1.12 | -1.78 | 147.69 | 11.33 | 234.05 | 0.2437 | -605.0 | -675.3 | |
| 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. | |