| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.05 | 79.07 | 30.77 | 67.59 | -9.38 | 194.31 | 52.22 | 253.01 | 0.8171 | 8.4 | 250.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.54 | 1.61 | 0.48 | 1.44 | -9.07 | 196.37 | 54.28 | 254.04 | 0.8360 | 80.7 | 60.4 | |
| 12.76 | 37.21 | 11.43 | 33.02 | -9.55 | 196.17 | 54.07 | 253.42 | 0.8353 | 396.3 | 487.8 | |
| 4.28 | -2.00 | 3.78 | -2.00 | -9.28 | 195.63 | 53.54 | 253.57 | 0.8297 | 748.0 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.94 | -8.66 | 195.45 | 53.36 | 254.23 | 0.8264 | 551.0 | 425.6 | |
| 0.27 | -2.00 | 0.23 | -2.00 | -9.10 | 195.13 | 53.04 | 253.62 | 0.8245 | 610.0 | 999999 | |
| 0.00 | 0.98 | 0.00 | 0.85 | -9.83 | 194.94 | 52.84 | 252.70 | 0.8246 | 225.0 | 216.6 | |
| 0.00 | 0.54 | 0.00 | 0.46 | -9.58 | 194.62 | 52.53 | 252.89 | 0.8210 | 177.0 | 192.2 | |
| 0.00 | 1.70 | 0.00 | 1.43 | -8.47 | 193.85 | 51.75 | 253.95 | 0.8104 | 224.0 | 166.3 | |
| 0.00 | 3.93 | 0.00 | 3.30 | -9.68 | 193.50 | 51.40 | 252.39 | 0.8105 | 235.0 | 216.0 | |
| 0.00 | 0.27 | 0.00 | 0.22 | -9.18 | 192.90 | 50.81 | 252.78 | 0.8032 | -174.0 | -75.3 | |
| 0.00 | 0.98 | 0.00 | 0.79 | -8.44 | 192.09 | 49.99 | 253.39 | 0.7929 | -485.0 | -389.0 | |
| 18.20 | 29.53 | 14.85 | 24.13 | -9.36 | 192.16 | 50.07 | 252.31 | 0.7964 | -539.1 | -21.5 | |
| 0.00 | 1.25 | 0.00 | 1.01 | -8.93 | 191.99 | 49.89 | 252.76 | 0.7933 | -632.0 | -507.0 | |
| 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. | |