| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.46 | 247.56 | 126.74 | 505.17 | 15.48 | 9.92 | -76.46 | 75.01 | 0.9686 | 194.3 | 129.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.55 | 0.00 | 2.69 | 18.76 | 12.54 | -73.84 | 71.61 | 0.9597 | -229.0 | -153.6 | |
| 17.88 | 101.15 | 26.66 | 151.42 | 14.82 | 15.38 | -71.00 | 75.69 | 0.9448 | -516.3 | -163.7 | |
| 0.00 | 0.69 | 0.00 | 1.36 | 19.09 | 10.39 | -75.99 | 71.31 | 0.9691 | 462.0 | 397.5 | |
| 0.00 | 0.78 | 0.00 | 1.45 | 14.79 | 11.22 | -75.16 | 75.75 | 0.9655 | 403.0 | 452.7 | |
| 1.64 | 113.33 | 3.13 | 251.84 | 14.74 | 10.90 | -75.48 | 75.80 | 0.9669 | 383.2 | 310.4 | |
| 1.81 | -5.00 | 3.43 | -5.00 | 14.56 | 10.96 | -75.42 | 75.99 | 0.9666 | 461.3 | 999999 | |
| 0.00 | 1.38 | 0.00 | 2.72 | 15.11 | 10.38 | -76.00 | 75.42 | 0.9690 | 432.0 | 356.8 | |
| 0.00 | 0.26 | 0.00 | 0.57 | 16.51 | 8.66 | -77.72 | 73.97 | 0.9757 | 317.0 | 313.3 | |
| 6.22 | -5.00 | 12.65 | -5.00 | 14.98 | 9.86 | -76.52 | 75.55 | 0.9712 | 582.4 | 999999 | |
| 7.17 | -5.00 | 14.34 | -5.00 | 14.39 | 10.24 | -76.14 | 76.16 | 0.9696 | 217.6 | 999999 | |
| 21.42 | -5.00 | 51.56 | -5.00 | 15.89 | 7.68 | -78.70 | 74.60 | 0.9792 | 406.0 | 999999 | |
| 0.00 | 0.52 | 0.00 | 1.49 | 16.92 | 5.60 | -80.78 | 73.51 | 0.9857 | 279.0 | 273.2 | |
| 4.32 | 14.34 | 14.97 | 49.78 | 17.17 | 3.73 | -82.65 | 73.21 | 0.9904 | 239.5 | 136.4 | |
| 0.00 | 13.56 | 0.00 | 41.85 | 15.94 | 4.81 | -81.57 | 74.49 | 0.9879 | 305.0 | 252.0 | |
| 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. | |