| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.52 | 29.56 | 4.95 | 20.10 | -14.90 | 248.43 | -37.49 | 120.78 | 0.6860 | -199.8 | -314.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.74 | 10.89 | 1.80 | 7.12 | -15.50 | 251.60 | -34.32 | 123.71 | 0.6554 | 770.7 | 597.0 | |
| 4.16 | -1.00 | 2.72 | -1.00 | -15.27 | 251.57 | -34.35 | 123.39 | 0.6542 | 875.3 | 999999 | |
| 0.00 | 1.68 | 0.00 | 1.08 | -13.75 | 251.76 | -34.15 | 121.49 | 0.6418 | 498.0 | 521.3 | |
| 0.00 | 2.21 | 0.00 | 1.52 | -13.99 | 247.24 | -38.68 | 118.74 | 0.6939 | -704.0 | -611.8 | |
| 0.00 | 2.04 | 0.00 | 1.40 | -14.10 | 247.06 | -38.86 | 118.77 | 0.6965 | -583.0 | -549.0 | |
| 0.00 | 1.42 | 0.00 | 0.98 | -14.07 | 246.66 | -39.25 | 118.48 | 0.7006 | -628.0 | -553.0 | |
| 0.62 | 2.83 | 0.43 | 1.97 | -14.44 | 246.46 | -39.45 | 118.84 | 0.7048 | -794.1 | -640.4 | |
| 0.00 | 1.15 | 0.00 | 0.81 | -14.80 | 246.30 | -39.61 | 119.21 | 0.7085 | -574.0 | -546.2 | |
| 0.00 | 1.24 | 0.00 | 0.88 | -15.66 | 246.07 | -39.85 | 120.14 | 0.7158 | -685.0 | -607.9 | |
| 0.00 | 1.68 | 0.00 | 1.19 | -15.68 | 245.81 | -40.10 | 120.02 | 0.7185 | -714.0 | -552.1 | |
| 0.00 | 0.27 | 0.00 | 0.19 | -15.52 | 245.81 | -40.10 | 119.81 | 0.7177 | -608.0 | -577.7 | |
| 0.00 | 2.12 | 0.00 | 1.51 | -14.93 | 245.50 | -40.42 | 118.89 | 0.7178 | -830.0 | -724.8 | |
| 0.00 | 0.97 | 0.00 | 0.69 | -15.24 | 245.30 | -40.61 | 119.16 | 0.7215 | -538.0 | -556.1 | |
| 0.00 | 1.06 | 0.00 | 0.76 | -15.21 | 244.90 | -41.02 | 118.88 | 0.7256 | -653.0 | -568.4 | |
| 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. | |