| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.58 | 46.83 | 10.57 | 24.02 | -15.81 | 113.90 | 2.21 | 187.82 | 0.2600 | -305.6 | -169.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.89 | 4.33 | 1.49 | 2.23 | -15.64 | 118.45 | 6.76 | 204.35 | 0.2761 | 962.0 | 742.5 | |
| 0.00 | 2.53 | 0.00 | 1.30 | -15.61 | 118.10 | 6.41 | 203.28 | 0.2733 | 921.0 | 720.5 | |
| 0.00 | 2.26 | 0.00 | 1.17 | -17.53 | 117.82 | 6.12 | 199.81 | 0.3013 | 764.0 | 667.7 | |
| 0.00 | 1.62 | 0.00 | 0.83 | -15.11 | 116.51 | 4.81 | 198.55 | 0.2558 | 1093.0 | 782.9 | |
| 0.00 | 0.90 | 0.00 | 0.47 | -16.90 | 116.20 | 4.51 | 195.47 | 0.2831 | 781.0 | 678.5 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -15.89 | 115.86 | 4.17 | 195.34 | 0.2653 | 869.0 | 631.3 | |
| 0.00 | 0.72 | 0.00 | 0.37 | -17.16 | 114.58 | 2.89 | 189.90 | 0.2813 | 724.0 | 547.4 | |
| 0.00 | 1.26 | 0.00 | 0.65 | -15.80 | 113.65 | 1.95 | 187.38 | 0.2563 | -820.0 | -636.9 | |
| 0.00 | 1.35 | 0.00 | 0.69 | -15.30 | 113.39 | 1.70 | 186.65 | 0.2474 | -783.0 | -607.7 | |
| 1.90 | 12.73 | 0.97 | 6.52 | -15.99 | 112.86 | 1.16 | 184.36 | 0.2582 | -966.5 | -886.5 | |
| 4.42 | -10.00 | 2.27 | -10.00 | -15.90 | 112.57 | 0.88 | 183.31 | 0.2562 | -1194.7 | 999999 | |
| 11.37 | 14.98 | 5.84 | 7.69 | -16.31 | 112.54 | 0.85 | 183.11 | 0.2631 | -1003.3 | -643.5 | |
| 0.00 | 1.90 | 0.00 | 0.96 | -12.71 | 111.13 | -0.57 | 177.25 | 0.2017 | -947.0 | -706.6 | |
| 0.00 | 1.35 | 0.00 | 0.68 | -11.26 | 109.64 | -2.05 | 168.71 | 0.1800 | -813.0 | -597.9 | |
| 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. | |