| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.78 | 32.17 | 5.03 | 20.58 | -19.79 | 35.23 | -38.07 | 113.37 | 0.6339 | 86.4 | 10.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.71 | 4.79 | 1.06 | 2.96 | -19.45 | 37.92 | -35.38 | 113.89 | 0.5994 | 854.9 | 661.2 | |
| 0.00 | 2.05 | 0.00 | 1.28 | -19.47 | 37.37 | -35.93 | 113.70 | 0.6065 | 770.0 | 604.5 | |
| 0.00 | 1.28 | 0.00 | 0.80 | -19.28 | 37.19 | -36.11 | 113.31 | 0.6081 | 656.0 | 540.1 | |
| 2.48 | 4.02 | 1.54 | 2.50 | -18.94 | 37.12 | -36.18 | 112.74 | 0.6078 | 825.5 | 725.2 | |
| 0.00 | 2.14 | 0.00 | 1.34 | -19.07 | 36.78 | -36.53 | 112.82 | 0.6126 | 444.0 | 323.6 | |
| 0.00 | 0.77 | 0.00 | 0.49 | -19.07 | 35.83 | -37.47 | 112.46 | 0.6245 | 424.0 | 307.9 | |
| 0.00 | 4.45 | 0.00 | 2.85 | -19.72 | 35.14 | -38.17 | 113.22 | 0.6353 | -658.0 | -676.7 | |
| 0.00 | 2.91 | 0.00 | 1.87 | -19.26 | 34.62 | -38.68 | 112.33 | 0.6402 | -633.0 | -450.4 | |
| 0.00 | 1.11 | 0.00 | 0.72 | -19.82 | 34.30 | -39.00 | 113.07 | 0.6459 | -501.0 | -355.4 | |
| 0.00 | 0.94 | 0.00 | 0.61 | -19.11 | 34.22 | -39.08 | 111.97 | 0.6447 | -725.0 | -519.2 | |
| 0.00 | 1.03 | 0.00 | 0.66 | -18.79 | 34.11 | -39.19 | 111.46 | 0.6451 | -859.0 | -717.8 | |
| 1.71 | 2.74 | 1.14 | 1.82 | -21.18 | 32.68 | -40.62 | 114.53 | 0.6697 | 663.3 | 522.0 | |
| 0.00 | 1.20 | 0.00 | 0.80 | -21.35 | 32.07 | -41.23 | 114.57 | 0.6773 | 381.0 | 299.6 | |
| 1.88 | 2.74 | 1.29 | 1.88 | -21.77 | 30.55 | -42.75 | 114.66 | 0.6961 | -724.3 | -610.4 | |
| 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. | |