| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.98 | 210.64 | 73.54 | 374.94 | 15.60 | 278.92 | -74.45 | 75.30 | 0.9592 | -121.5 | 15.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.62 | 152.97 | 13.21 | 245.29 | 15.76 | 281.48 | -71.89 | 75.19 | 0.9476 | -591.7 | -12.6 | |
| 4.36 | -1.00 | 6.91 | -1.00 | 16.19 | 280.78 | -72.59 | 74.73 | 0.9513 | -240.6 | 999999 | |
| 1.22 | -1.00 | 1.93 | -1.00 | 15.70 | 280.81 | -72.56 | 75.25 | 0.9511 | 75.1 | 999999 | |
| 0.26 | -1.00 | 0.41 | -1.00 | 15.76 | 280.76 | -72.61 | 75.19 | 0.9514 | -105.7 | 999999 | |
| 12.72 | -1.00 | 20.28 | -1.00 | 15.13 | 280.69 | -72.68 | 75.84 | 0.9518 | -374.7 | 999999 | |
| 4.44 | -1.00 | 7.26 | -1.00 | 15.03 | 280.24 | -73.13 | 75.94 | 0.9541 | 157.8 | 999999 | |
| 4.70 | 25.87 | 8.55 | 46.41 | 16.72 | 278.30 | -75.07 | 74.15 | 0.9632 | 408.2 | 399.6 | |
| 0.00 | 1.05 | 0.00 | 1.89 | 16.38 | 278.32 | -75.05 | 74.50 | 0.9632 | 102.0 | 100.9 | |
| 0.00 | 0.96 | 0.00 | 1.72 | 14.78 | 278.54 | -74.83 | 76.16 | 0.9624 | 443.0 | 446.6 | |
| 0.00 | 3.66 | 0.00 | 8.81 | 15.66 | 274.26 | -79.11 | 75.11 | 0.9793 | 360.0 | 293.8 | |
| 0.00 | 1.22 | 0.00 | 2.15 | 11.02 | 279.01 | -74.36 | 80.09 | 0.9608 | 78.0 | 51.8 | |
| 4.88 | 24.91 | 12.89 | 68.67 | 15.49 | 273.10 | -80.27 | 75.23 | 0.9831 | 170.0 | -217.2 | |
| 0.78 | -12.00 | 2.10 | -12.00 | 15.26 | 272.92 | -80.46 | 75.46 | 0.9837 | -129.6 | 999999 | |
| 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. | |