| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.54 | 55.33 | 18.05 | 44.69 | 9.61 | 146.99 | 52.75 | 276.56 | 0.7917 | 273.4 | -35.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.34 | 3.21 | 1.20 | 2.87 | 9.88 | 151.25 | 57.01 | 277.08 | 0.8348 | -445.9 | -279.0 | |
| 0.00 | 1.78 | 0.00 | 1.59 | 10.64 | 151.30 | 57.05 | 278.00 | 0.8350 | -496.0 | -381.5 | |
| 3.65 | 12.83 | 3.08 | 10.78 | 10.28 | 148.83 | 54.59 | 277.48 | 0.8110 | -575.6 | -565.1 | |
| 0.80 | -3.00 | 0.67 | -3.00 | 10.43 | 148.55 | 54.31 | 277.66 | 0.8081 | -645.9 | 999999 | |
| 0.00 | 0.89 | 0.00 | 0.73 | 9.53 | 147.81 | 53.56 | 276.51 | 0.8008 | -582.0 | -519.7 | |
| 0.00 | 0.98 | 0.00 | 0.80 | 9.12 | 147.71 | 53.47 | 275.98 | 0.7999 | -450.0 | -418.8 | |
| 0.00 | 1.34 | 0.00 | 1.09 | 9.75 | 147.49 | 53.25 | 276.77 | 0.7975 | -570.0 | -563.1 | |
| 0.00 | 5.79 | 0.00 | 4.60 | 8.91 | 146.15 | 51.90 | 275.64 | 0.7835 | 488.0 | 335.9 | |
| 0.00 | 0.89 | 0.00 | 0.70 | 10.20 | 145.98 | 51.74 | 277.30 | 0.7813 | 323.0 | 240.4 | |
| 16.75 | 22.45 | 13.10 | 17.56 | 9.25 | 145.47 | 51.23 | 276.05 | 0.7761 | 735.5 | 474.8 | |
| 0.00 | 1.43 | 0.00 | 1.11 | 9.98 | 145.48 | 51.24 | 277.00 | 0.7760 | 528.0 | 411.6 | |
| 0.00 | 1.43 | 0.00 | 1.11 | 10.10 | 145.46 | 51.22 | 277.16 | 0.7757 | 566.0 | 415.9 | |
| 0.00 | 0.80 | 0.00 | 0.61 | 10.28 | 144.24 | 49.99 | 277.37 | 0.7622 | 440.0 | 364.7 | |
| 0.00 | 1.51 | 0.00 | 1.14 | 7.99 | 143.65 | 49.41 | 274.32 | 0.7564 | 527.0 | 395.2 | |
| 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. | |