| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.44 | 227.04 | 35.49 | 187.55 | -13.34 | 229.54 | 52.54 | 254.89 | 0.8019 | 429.1 | 207.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.55 | 208.14 | 20.60 | 173.90 | -12.88 | 230.35 | 53.35 | 255.69 | 0.8094 | 873.6 | 273.5 | |
| 17.89 | -1.00 | 14.89 | -1.00 | -13.42 | 229.89 | 52.90 | 254.95 | 0.8055 | 826.5 | 999999 | |
| 0.00 | 3.33 | 0.00 | 2.64 | -11.50 | 227.93 | 50.94 | 257.08 | 0.7829 | -379.0 | -350.7 | |
| 0.00 | 0.81 | 0.00 | 0.64 | -10.86 | 227.68 | 50.68 | 257.86 | 0.7794 | -487.0 | -394.6 | |
| 0.00 | 0.63 | 0.00 | 0.50 | -11.17 | 227.70 | 50.71 | 257.47 | 0.7800 | -385.0 | -440.7 | |
| 0.00 | 1.35 | 0.00 | 1.06 | -11.54 | 227.69 | 50.70 | 257.00 | 0.7804 | -608.0 | -562.2 | |
| 0.00 | 0.72 | 0.00 | 0.54 | -13.04 | 224.96 | 47.97 | 254.59 | 0.7529 | -605.0 | -433.4 | |
| 0.00 | 0.90 | 0.00 | 0.68 | -14.56 | 224.91 | 47.91 | 252.58 | 0.7551 | -416.0 | -370.6 | |
| 0.00 | 0.99 | 0.00 | 0.73 | -14.16 | 223.73 | 46.73 | 252.85 | 0.7412 | -669.0 | -594.8 | |
| 0.00 | 1.35 | 0.00 | 0.98 | -12.90 | 223.18 | 46.19 | 254.42 | 0.7326 | -627.0 | -413.3 | |
| 0.00 | 1.26 | 0.00 | 0.86 | -20.31 | 217.65 | 40.65 | 242.47 | 0.6912 | -501.0 | -363.1 | |
| 0.00 | 0.81 | 0.00 | 0.54 | -21.73 | 215.94 | 38.94 | 239.71 | 0.6785 | -684.0 | -571.9 | |
| 0.00 | 0.27 | 0.00 | 0.18 | -22.21 | 216.10 | 39.10 | 239.13 | 0.6826 | -605.0 | -545.7 | |
| 0.00 | 1.44 | 0.00 | 0.97 | -22.50 | 216.11 | 39.11 | 238.74 | 0.6841 | -500.0 | -392.2 | |
| 0.00 | 2.88 | 0.00 | 1.93 | -21.51 | 215.70 | 38.70 | 239.89 | 0.6748 | -755.0 | -519.4 | |
| 0.00 | 1.08 | 0.00 | 0.72 | -22.30 | 215.11 | 38.12 | 238.49 | 0.6722 | -671.0 | -558.6 | |
| 0.00 | 1.08 | 0.00 | 0.68 | -22.85 | 210.41 | 33.42 | 234.85 | 0.6229 | -748.0 | -638.8 | |
| 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. | |