| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.49 | 56.51 | 12.49 | 31.22 | -19.75 | 51.04 | 18.47 | 222.35 | 0.4438 | 288.2 | 195.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.08 | 0.00 | 0.60 | -18.72 | 53.83 | 21.27 | 228.34 | 0.4617 | 813.0 | 623.0 | |
| 16.89 | 28.53 | 9.44 | 15.94 | -19.27 | 53.63 | 21.06 | 227.16 | 0.4646 | 981.5 | 653.8 | |
| 0.00 | 1.72 | 0.00 | 0.95 | -18.92 | 51.90 | 19.34 | 225.42 | 0.4416 | 830.0 | 649.8 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -19.66 | 51.89 | 19.33 | 224.16 | 0.4492 | 772.0 | 625.3 | |
| 0.00 | 1.72 | 0.00 | 0.95 | -20.66 | 50.92 | 18.36 | 221.14 | 0.4498 | 816.0 | 669.3 | |
| 0.00 | 3.79 | 0.00 | 2.09 | -20.40 | 50.55 | 17.98 | 220.98 | 0.4431 | 718.0 | 700.2 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -19.86 | 49.84 | 17.27 | 220.76 | 0.4296 | -742.0 | -591.1 | |
| 0.00 | 2.44 | 0.00 | 1.33 | -19.61 | 48.87 | 16.30 | 219.59 | 0.4167 | -992.0 | -831.9 | |
| 5.60 | 7.58 | 3.05 | 4.13 | -19.80 | 48.62 | 16.05 | 218.86 | 0.4165 | -1053.1 | -753.7 | |
| 0.00 | 1.08 | 0.00 | 0.60 | -22.13 | 48.50 | 15.94 | 215.15 | 0.4435 | 626.0 | 562.8 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -19.55 | 46.35 | 13.79 | 215.18 | 0.3915 | -782.0 | -661.9 | |
| 0.00 | 1.99 | 0.00 | 1.07 | -19.68 | 45.83 | 13.27 | 213.98 | 0.3884 | -725.0 | -564.2 | |
| 0.00 | 3.70 | 0.00 | 1.99 | -22.47 | 41.03 | 8.46 | 200.37 | 0.3924 | -618.0 | -569.5 | |
| 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. | |