| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 55.30 | 0.00 | 27.92 | -12.73 | 298.35 | -7.56 | 137.62 | 0.1806 | 1.7 | -107.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.30 | 0.00 | 0.65 | -6.69 | 311.77 | 5.86 | 274.41 | 0.1022 | 1005.0 | 818.1 | |
| 0.00 | 1.13 | 0.00 | 0.56 | -12.59 | 309.50 | 3.60 | 212.95 | 0.1132 | 815.0 | 637.2 | |
| 0.00 | 0.87 | 0.00 | 0.43 | -14.51 | 308.85 | 2.95 | 201.29 | 0.1379 | 846.0 | 720.5 | |
| 0.00 | 1.83 | 0.00 | 0.91 | -10.12 | 307.38 | 1.48 | 206.36 | 0.0576 | 903.0 | 803.3 | |
| 0.00 | 0.61 | 0.00 | 0.31 | -16.45 | 306.64 | 0.74 | 184.37 | 0.1623 | 874.0 | 766.6 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -16.69 | 305.21 | -0.69 | 175.98 | 0.1664 | 747.0 | 582.7 | |
| 0.00 | 2.17 | 0.00 | 1.08 | -11.64 | 303.77 | -2.13 | 154.90 | 0.0863 | 1113.0 | 873.6 | |
| 0.00 | 0.96 | 0.00 | 0.48 | -12.26 | 303.76 | -2.14 | 157.66 | 0.0964 | 843.0 | 691.4 | |
| 0.00 | 0.87 | 0.00 | 0.43 | -11.13 | 303.68 | -2.22 | 151.14 | 0.0791 | 945.0 | 725.8 | |
| 0.00 | 2.09 | 0.00 | 1.04 | -11.49 | 303.59 | -2.31 | 152.25 | 0.0854 | 1077.0 | 834.8 | |
| 0.00 | 0.96 | 0.00 | 0.48 | -12.56 | 303.58 | -2.33 | 157.14 | 0.1024 | 828.0 | 596.8 | |
| 0.00 | 1.22 | 0.00 | 0.61 | -12.23 | 303.52 | -2.38 | 155.27 | 0.0976 | 885.0 | 704.2 | |
| 0.00 | 1.48 | 0.00 | 0.73 | -11.72 | 303.46 | -2.44 | 152.30 | 0.0901 | 799.0 | 655.2 | |
| 0.00 | 2.35 | 0.00 | 1.17 | -11.15 | 303.29 | -2.62 | 147.21 | 0.0831 | 517.0 | 657.6 | |
| 0.00 | 0.26 | 0.00 | 0.13 | -12.17 | 303.12 | -2.78 | 151.47 | 0.0997 | 701.0 | 556.3 | |
| 0.00 | 1.39 | 0.00 | 0.69 | -11.00 | 302.89 | -3.01 | 142.39 | 0.0848 | 779.0 | 627.3 | |
| 0.00 | 1.65 | 0.00 | 0.83 | -15.87 | 298.50 | -7.40 | 140.82 | 0.1971 | 648.0 | 510.5 | |
| 0.00 | 1.39 | 0.00 | 0.70 | -1.96 | 298.13 | -7.77 | 56.39 | 0.1629 | 985.0 | 793.2 | |
| 0.00 | 2.52 | 0.00 | 1.27 | -12.25 | 297.79 | -8.11 | 123.03 | 0.1653 | -881.0 | -730.6 | |
| 0.00 | 1.22 | 0.00 | 0.61 | -8.73 | 296.42 | -9.48 | 100.03 | 0.1661 | -835.0 | -746.1 | |
| 0.00 | 1.04 | 0.00 | 0.53 | -13.37 | 295.33 | -10.57 | 121.62 | 0.2106 | -923.0 | -779.6 | |
| 0.00 | 1.48 | 0.00 | 0.75 | -13.25 | 295.24 | -10.66 | 120.91 | 0.2108 | -935.0 | -799.8 | |
| 0.00 | 1.56 | 0.00 | 0.79 | -8.97 | 295.25 | -10.65 | 100.38 | 0.1865 | -687.0 | -603.9 | |
| 0.00 | 2.26 | 0.00 | 1.15 | -13.89 | 294.71 | -11.19 | 122.33 | 0.2240 | -843.0 | -678.2 | |
| 0.00 | 1.48 | 0.00 | 0.75 | -14.85 | 294.41 | -11.49 | 125.21 | 0.2368 | -986.0 | -722.7 | |
| 0.00 | 1.04 | 0.00 | 0.53 | -15.45 | 294.34 | -11.56 | 127.15 | 0.2434 | -718.0 | -599.2 | |
| 0.00 | 1.22 | 0.00 | 0.62 | -14.84 | 294.10 | -11.81 | 124.49 | 0.2411 | -803.0 | -740.3 | |
| 0.00 | 1.13 | 0.00 | 0.57 | -8.43 | 294.07 | -11.83 | 96.91 | 0.2053 | -866.0 | -688.2 | |
| 0.00 | 4.95 | 0.00 | 2.54 | -15.70 | 293.60 | -12.30 | 126.36 | 0.2558 | -650.0 | -596.9 | |
| 0.00 | 1.39 | 0.00 | 0.70 | -7.98 | 293.81 | -12.10 | 94.62 | 0.2092 | -937.0 | -778.1 | |
| 0.00 | 1.48 | 0.00 | 0.75 | -11.95 | 293.59 | -12.31 | 112.39 | 0.2267 | -825.0 | -643.3 | |
| 0.00 | 2.78 | 0.00 | 1.43 | -15.57 | 293.36 | -12.55 | 125.43 | 0.2580 | -1073.0 | -891.2 | |
| 0.00 | 2.35 | 0.00 | 1.21 | -15.64 | 292.37 | -13.54 | 123.72 | 0.2722 | -940.0 | -761.9 | |
| 0.00 | 1.48 | 0.00 | 0.76 | -15.78 | 292.07 | -13.83 | 123.63 | 0.2776 | -771.0 | -583.4 | |
| 0.00 | 0.96 | 0.00 | 0.49 | -14.28 | 291.47 | -14.43 | 117.84 | 0.2743 | -771.0 | -671.2 | |
| 0.00 | 1.39 | 0.00 | 0.72 | -16.39 | 291.26 | -14.65 | 124.05 | 0.2941 | -806.0 | -696.1 | |
| 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. | |