| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.77 | 344.51 | 38.08 | 179.61 | 16.35 | 25.02 | -15.27 | 54.99 | 0.3067 | -99.9 | -47.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.34 | 178.98 | 16.56 | 91.67 | 15.91 | 28.50 | -11.79 | 50.66 | 0.2551 | -1371.6 | -412.8 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 16.65 | 27.42 | -12.87 | 50.76 | 0.2767 | -731.0 | -479.8 | |
| 5.04 | 9.28 | 2.60 | 4.78 | 16.25 | 27.32 | -12.97 | 52.16 | 0.2741 | -1092.0 | -623.5 | |
| 0.00 | 11.17 | 0.00 | 5.78 | 16.25 | 25.95 | -14.34 | 54.76 | 0.2924 | -1045.0 | -877.6 | |
| 0.00 | 1.53 | 0.00 | 0.80 | 17.01 | 25.70 | -14.59 | 53.05 | 0.3028 | -834.0 | -720.2 | |
| 1.35 | 2.88 | 0.70 | 1.50 | 16.42 | 25.67 | -14.61 | 54.73 | 0.2977 | -1035.9 | -799.6 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 16.14 | 25.30 | -14.98 | 56.18 | 0.3003 | -681.0 | -546.8 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 16.50 | 25.21 | -15.08 | 55.29 | 0.3047 | -909.0 | -730.4 | |
| 0.00 | 2.34 | 0.00 | 1.22 | 16.69 | 25.13 | -15.16 | 54.92 | 0.3074 | -917.0 | -724.2 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 16.22 | 25.04 | -15.25 | 56.37 | 0.3047 | -830.0 | -643.8 | |
| 0.00 | 2.61 | 0.00 | 1.36 | 16.74 | 24.73 | -15.56 | 55.43 | 0.3133 | -719.0 | -606.6 | |
| 0.00 | 0.63 | 0.00 | 0.33 | 16.39 | 24.56 | -15.73 | 56.64 | 0.3127 | -751.0 | -556.0 | |
| 0.00 | 1.62 | 0.00 | 0.85 | 16.50 | 24.09 | -16.20 | 57.05 | 0.3201 | -871.0 | -753.7 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 15.79 | 23.99 | -16.30 | 59.18 | 0.3159 | -819.0 | -680.4 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 16.14 | 21.54 | -18.75 | 61.36 | 0.3533 | 963.0 | 760.1 | |
| 3.24 | 8.74 | 1.72 | 4.64 | 16.84 | 21.37 | -18.92 | 59.78 | 0.3607 | 1155.1 | 847.8 | |
| 1.17 | -16.00 | 0.62 | -16.00 | 17.02 | 21.22 | -19.07 | 59.51 | 0.3641 | 984.5 | 999999 | |
| 0.00 | 1.53 | 0.00 | 0.82 | 18.81 | 20.91 | -19.37 | 55.64 | 0.3820 | 834.0 | 631.4 | |
| 2.34 | 6.58 | 1.24 | 3.49 | 16.28 | 21.06 | -19.23 | 61.56 | 0.3611 | 1120.5 | 858.3 | |
| 0.00 | 1.53 | 0.00 | 0.82 | 18.15 | 20.85 | -19.43 | 57.22 | 0.3776 | 731.0 | 648.4 | |
| 0.00 | 0.72 | 0.00 | 0.39 | 18.68 | 20.73 | -19.56 | 56.17 | 0.3835 | 837.0 | 684.0 | |
| 0.00 | 1.44 | 0.00 | 0.77 | 18.61 | 20.56 | -19.72 | 56.52 | 0.3851 | 819.0 | 682.4 | |
| 1.17 | 23.69 | 0.62 | 12.63 | 17.22 | 20.69 | -19.60 | 59.64 | 0.3729 | 1031.3 | 768.0 | |
| 0.00 | 1.08 | 0.00 | 0.58 | 18.98 | 20.45 | -19.84 | 55.82 | 0.3895 | 582.0 | 423.8 | |
| 0.00 | 2.70 | 0.00 | 1.45 | 17.96 | 20.54 | -19.75 | 58.06 | 0.3804 | 1035.0 | 865.7 | |
| 2.25 | 4.32 | 1.20 | 2.30 | 15.98 | 20.62 | -19.67 | 62.77 | 0.3655 | 984.8 | 827.6 | |
| 0.00 | 2.61 | 0.00 | 1.40 | 17.82 | 20.18 | -20.11 | 58.79 | 0.3843 | 849.0 | 654.8 | |
| 0.00 | 2.07 | 0.00 | 1.11 | 17.60 | 20.10 | -20.18 | 59.39 | 0.3838 | 837.0 | 632.0 | |
| 0.00 | 1.35 | 0.00 | 0.73 | 20.57 | 19.69 | -20.60 | 53.30 | 0.4125 | 788.0 | 533.3 | |
| 1.53 | 18.92 | 0.82 | 10.12 | 17.10 | 20.06 | -20.23 | 60.61 | 0.3809 | 1012.9 | 814.6 | |
| 0.00 | 1.53 | 0.00 | 0.82 | 17.37 | 19.72 | -20.56 | 60.34 | 0.3874 | 773.0 | 540.2 | |
| 0.00 | 1.89 | 0.00 | 1.02 | 17.03 | 19.66 | -20.63 | 61.21 | 0.3860 | 954.0 | 810.5 | |
| 9.10 | 24.86 | 4.88 | 13.32 | 16.15 | 19.45 | -20.83 | 63.51 | 0.3833 | 1122.4 | 593.9 | |
| 10.27 | 14.86 | 5.52 | 7.99 | 16.92 | 19.30 | -20.99 | 61.83 | 0.3903 | 948.5 | 530.1 | |
| 2.97 | 5.76 | 1.60 | 3.10 | 16.23 | 18.97 | -21.32 | 63.79 | 0.3907 | 831.4 | 703.7 | |
| 0.00 | 1.08 | 0.00 | 0.58 | 16.78 | 18.87 | -21.41 | 62.58 | 0.3955 | 498.0 | 308.5 | |
| 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. | |