| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.69 | 30.92 | 1.87 | 15.76 | -8.50 | 8.98 | -12.86 | 101.18 | 0.2263 | 379.8 | 203.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.23 | 0.00 | 0.62 | -6.85 | 12.58 | -9.26 | 94.07 | 0.1609 | 997.0 | 848.3 | |
| 0.00 | 2.02 | 0.00 | 1.02 | -8.97 | 12.22 | -9.62 | 106.38 | 0.1728 | 849.0 | 654.0 | |
| 0.00 | 0.79 | 0.00 | 0.40 | -7.71 | 12.19 | -9.65 | 99.08 | 0.1689 | 905.0 | 754.9 | |
| 0.00 | 1.41 | 0.00 | 0.71 | -6.02 | 11.64 | -10.19 | 89.10 | 0.1768 | 794.0 | 659.2 | |
| 0.00 | 2.02 | 0.00 | 1.02 | -8.06 | 11.41 | -10.42 | 100.37 | 0.1829 | 969.0 | 728.4 | |
| 0.00 | 1.05 | 0.00 | 0.53 | -7.32 | 10.48 | -11.36 | 95.91 | 0.1973 | 834.0 | 604.7 | |
| 0.00 | 1.05 | 0.00 | 0.53 | -9.71 | 10.25 | -11.59 | 107.41 | 0.2084 | 458.0 | 313.7 | |
| 0.00 | 1.05 | 0.00 | 0.53 | -8.96 | 10.18 | -11.65 | 103.79 | 0.2064 | -756.0 | -584.4 | |
| 3.69 | 5.63 | 1.87 | 2.85 | -9.85 | 9.71 | -12.12 | 107.36 | 0.2178 | 1146.3 | 849.2 | |
| 0.00 | 1.49 | 0.00 | 0.76 | -8.83 | 9.75 | -12.08 | 102.77 | 0.2131 | 773.0 | 548.5 | |
| 0.00 | 1.05 | 0.00 | 0.54 | -11.02 | 9.66 | -12.17 | 112.35 | 0.2247 | 810.0 | 606.8 | |
| 0.00 | 1.23 | 0.00 | 0.63 | -9.42 | 9.32 | -12.51 | 105.02 | 0.2223 | 802.0 | 684.1 | |
| 0.00 | 2.02 | 0.00 | 1.03 | -9.84 | 9.24 | -12.59 | 106.76 | 0.2253 | 776.0 | 620.4 | |
| 0.00 | 1.32 | 0.00 | 0.67 | -10.52 | 8.65 | -13.18 | 108.88 | 0.2380 | 697.0 | 513.3 | |
| 0.00 | 1.23 | 0.00 | 0.64 | -7.21 | 5.50 | -16.34 | 94.23 | 0.2811 | -990.0 | -791.6 | |
| 0.00 | 1.14 | 0.00 | 0.59 | -7.00 | 5.32 | -16.52 | 93.44 | 0.2840 | -923.0 | -760.3 | |
| 0.00 | 2.73 | 0.00 | 1.41 | -7.11 | 5.00 | -16.84 | 93.79 | 0.2894 | -991.0 | -761.9 | |
| 0.00 | 2.46 | 0.00 | 1.28 | -6.71 | 3.81 | -18.02 | 92.38 | 0.3089 | -980.0 | -788.8 | |
| 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. | |