| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.47 | 0.00 | 13.30 | -4.97 | 139.26 | -35.03 | 107.57 | 0.6022 | -716.5 | -600.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.76 | 0.00 | 1.08 | -4.19 | 140.14 | -34.15 | 106.79 | 0.5869 | -817.0 | -685.3 | |
| 0.00 | 2.02 | 0.00 | 1.24 | -3.93 | 140.01 | -34.28 | 106.29 | 0.5876 | -791.0 | -627.4 | |
| 0.00 | 1.67 | 0.00 | 1.02 | -4.03 | 139.79 | -34.50 | 106.35 | 0.5911 | -753.0 | -594.6 | |
| 0.00 | 1.14 | 0.00 | 0.70 | -4.96 | 139.70 | -34.59 | 107.79 | 0.5962 | -850.0 | -726.9 | |
| 0.00 | 1.06 | 0.00 | 0.65 | -4.70 | 139.42 | -34.87 | 107.23 | 0.5988 | -763.0 | -629.7 | |
| 0.00 | 3.34 | 0.00 | 2.07 | -4.92 | 139.26 | -35.03 | 107.51 | 0.6019 | -532.0 | -535.1 | |
| 0.00 | 0.97 | 0.00 | 0.61 | -6.66 | 138.98 | -35.31 | 110.07 | 0.6134 | -758.0 | -621.1 | |
| 0.00 | 1.94 | 0.00 | 1.20 | -3.96 | 139.13 | -35.16 | 105.90 | 0.5996 | -866.0 | -675.6 | |
| 0.00 | 1.41 | 0.00 | 0.88 | -6.05 | 138.96 | -35.33 | 109.11 | 0.6109 | -440.0 | -433.0 | |
| 0.00 | 0.88 | 0.00 | 0.55 | -6.23 | 138.94 | -35.35 | 109.39 | 0.6119 | -763.0 | -646.1 | |
| 0.00 | 2.46 | 0.00 | 1.54 | -6.45 | 138.89 | -35.40 | 109.70 | 0.6137 | -869.0 | -703.3 | |
| 0.00 | 0.53 | 0.00 | 0.33 | -5.87 | 138.90 | -35.39 | 108.80 | 0.6109 | -699.0 | -456.5 | |
| 0.00 | 0.97 | 0.00 | 0.60 | -5.45 | 138.74 | -35.55 | 108.07 | 0.6110 | -626.0 | -556.9 | |
| 0.00 | 1.32 | 0.00 | 0.83 | -3.83 | 137.91 | -36.38 | 105.12 | 0.6153 | -504.0 | -406.6 | |
| 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. | |