| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.47 | 63.56 | 6.95 | 32.90 | 18.88 | 241.95 | -11.30 | 39.68 | 0.2907 | 168.8 | 368.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 0.74 | 18.71 | 245.38 | -7.87 | 30.77 | 0.2545 | -747.0 | -574.1 | |
| 0.00 | 0.72 | 0.00 | 0.37 | 18.54 | 244.71 | -8.54 | 33.21 | 0.2582 | -814.0 | -663.1 | |
| 0.00 | 3.80 | 0.00 | 1.94 | 17.57 | 244.18 | -9.07 | 37.13 | 0.2502 | -328.0 | -405.2 | |
| 2.71 | 6.24 | 1.39 | 3.20 | 18.62 | 244.09 | -9.16 | 34.85 | 0.2652 | -1116.1 | -941.4 | |
| 4.61 | 5.97 | 2.37 | 3.06 | 18.31 | 243.78 | -9.47 | 36.46 | 0.2639 | -997.6 | -856.0 | |
| 0.00 | 1.90 | 0.00 | 0.98 | 18.90 | 243.68 | -9.57 | 35.38 | 0.2728 | -653.0 | -541.8 | |
| 1.72 | 3.80 | 0.89 | 1.97 | 19.59 | 242.33 | -10.92 | 37.38 | 0.2953 | -869.6 | -743.7 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 18.79 | 241.50 | -11.75 | 41.18 | 0.2941 | 928.0 | 836.5 | |
| 0.00 | 2.71 | 0.00 | 1.40 | 18.36 | 241.46 | -11.79 | 42.32 | 0.2892 | 1090.0 | 836.3 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 18.91 | 241.33 | -11.92 | 41.30 | 0.2974 | 899.0 | 744.3 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 18.51 | 241.26 | -11.99 | 42.43 | 0.2933 | 1055.0 | 811.1 | |
| 4.43 | 18.35 | 2.30 | 9.53 | 18.81 | 241.00 | -12.24 | 42.27 | 0.2998 | 1151.6 | 846.1 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 18.81 | 240.64 | -12.61 | 43.08 | 0.3038 | 711.0 | 617.7 | |
| 0.00 | 10.94 | 0.00 | 5.71 | 19.71 | 240.54 | -12.71 | 41.24 | 0.3156 | 752.0 | 803.3 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 19.30 | 240.34 | -12.91 | 42.59 | 0.3129 | 885.0 | 688.3 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 20.67 | 240.03 | -13.22 | 40.26 | 0.3326 | 850.0 | 566.1 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 18.47 | 239.81 | -13.44 | 45.63 | 0.3096 | 781.0 | 563.6 | |
| 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. | |