| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.82 | 113.14 | 37.64 | 132.10 | 18.79 | 171.42 | 63.39 | 290.74 | 0.9047 | -108.8 | 66.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.19 | 36.52 | 11.25 | 50.58 | 18.94 | 175.77 | 67.74 | 290.21 | 0.9344 | -447.4 | 28.2 | |
| 7.59 | 8.62 | 9.51 | 10.80 | 18.95 | 173.47 | 65.44 | 290.54 | 0.9203 | -517.8 | -300.6 | |
| 0.00 | 0.60 | 0.00 | 0.73 | 19.55 | 172.72 | 64.69 | 291.29 | 0.9161 | -307.0 | -384.7 | |
| 2.90 | 4.18 | 3.32 | 4.79 | 18.37 | 171.03 | 63.00 | 290.27 | 0.9033 | -314.4 | -226.1 | |
| 0.00 | 1.45 | 0.00 | 1.60 | 17.53 | 170.03 | 62.00 | 289.51 | 0.8951 | -289.0 | -279.3 | |
| 2.90 | 8.11 | 3.22 | 8.98 | 17.94 | 170.21 | 62.18 | 289.93 | 0.8969 | -453.9 | -400.3 | |
| 0.00 | 2.47 | 0.00 | 2.70 | 17.53 | 169.70 | 61.67 | 289.57 | 0.8927 | -707.0 | -590.3 | |
| 0.00 | 1.02 | 0.00 | 1.09 | 18.85 | 168.67 | 60.64 | 291.21 | 0.8867 | 183.0 | 124.5 | |
| 0.00 | 1.02 | 0.00 | 1.14 | 20.57 | 169.80 | 61.77 | 292.90 | 0.8974 | 286.0 | 233.2 | |
| 0.00 | 1.45 | 0.00 | 1.52 | 18.41 | 168.15 | 60.12 | 290.82 | 0.8821 | 257.0 | 93.2 | |
| 0.00 | 1.19 | 0.00 | 1.25 | 18.63 | 168.15 | 60.13 | 291.06 | 0.8825 | 152.0 | 140.6 | |
| 0.34 | 3.93 | 0.35 | 4.04 | 18.20 | 167.78 | 59.75 | 290.65 | 0.8789 | 236.8 | 275.9 | |
| 8.36 | 41.64 | 8.45 | 41.96 | 18.85 | 166.98 | 58.95 | 291.54 | 0.8737 | 699.4 | 264.6 | |
| 1.54 | -13.00 | 1.54 | -13.00 | 19.26 | 166.55 | 58.52 | 292.09 | 0.8709 | 726.9 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.92 | 20.30 | 165.48 | 57.45 | 293.50 | 0.8641 | 464.0 | 367.6 | |
| 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. | |