| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.42 | 151.33 | 21.26 | 81.55 | -16.00 | 249.10 | 2.24 | 185.38 | 0.3943 | -41.1 | -102.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.97 | 0.00 | 0.53 | -16.00 | 252.42 | 5.56 | 193.46 | 0.4017 | 799.0 | 638.5 | |
| 0.00 | 2.12 | 0.00 | 1.14 | -15.22 | 252.25 | 5.38 | 193.52 | 0.3888 | 998.0 | 751.6 | |
| 0.00 | 1.94 | 0.00 | 1.05 | -15.38 | 252.13 | 5.26 | 193.12 | 0.3909 | 999.0 | 855.3 | |
| 0.00 | 0.71 | 0.00 | 0.38 | -15.15 | 252.00 | 5.13 | 192.94 | 0.3868 | 773.0 | 601.5 | |
| 15.73 | 32.35 | 8.52 | 17.52 | -16.39 | 251.68 | 4.81 | 191.51 | 0.4051 | 1094.6 | 645.2 | |
| 2.30 | -5.00 | 1.25 | -5.00 | -16.65 | 251.50 | 4.63 | 190.96 | 0.4086 | 700.3 | 999999 | |
| 0.00 | 1.86 | 0.00 | 1.01 | -16.94 | 251.35 | 4.48 | 190.47 | 0.4128 | 938.0 | 747.6 | |
| 0.97 | 9.90 | 0.52 | 5.34 | -16.02 | 251.29 | 4.43 | 190.78 | 0.3982 | 1070.1 | 877.2 | |
| 0.00 | 2.83 | 0.00 | 1.54 | -17.37 | 251.26 | 4.39 | 190.09 | 0.4193 | 882.0 | 631.8 | |
| 0.97 | 4.24 | 0.53 | 2.32 | -17.56 | 250.89 | 4.02 | 189.16 | 0.4213 | 889.5 | 699.9 | |
| 0.00 | 3.09 | 0.00 | 1.67 | -15.85 | 250.45 | 3.58 | 188.82 | 0.3932 | 1166.0 | 906.5 | |
| 0.00 | 1.41 | 0.00 | 0.77 | -17.49 | 249.65 | 2.79 | 186.40 | 0.4174 | 874.0 | 608.9 | |
| 0.97 | 2.48 | 0.53 | 1.35 | -17.48 | 249.43 | 2.56 | 185.90 | 0.4170 | 958.4 | 666.0 | |
| 0.00 | 1.77 | 0.00 | 0.95 | -16.00 | 249.10 | 2.23 | 185.49 | 0.3929 | -513.0 | -317.8 | |
| 0.00 | 2.48 | 0.00 | 1.33 | -15.42 | 248.88 | 2.01 | 185.08 | 0.3831 | -662.0 | -496.6 | |
| 0.00 | 2.74 | 0.00 | 1.46 | -15.03 | 248.84 | 1.97 | 185.09 | 0.3768 | 1025.0 | 853.9 | |
| 3.71 | 20.24 | 1.99 | 10.87 | -15.54 | 248.57 | 1.70 | 184.27 | 0.3848 | -1116.1 | -721.9 | |
| 0.00 | 2.56 | 0.00 | 1.37 | -15.02 | 248.56 | 1.69 | 184.37 | 0.3764 | 439.0 | 327.9 | |
| 3.27 | -17.00 | 1.76 | -17.00 | -15.67 | 248.47 | 1.61 | 184.02 | 0.3868 | -1019.7 | 999999 | |
| 0.00 | 2.48 | 0.00 | 1.34 | -17.25 | 248.30 | 1.43 | 183.33 | 0.4118 | -991.0 | -771.9 | |
| 0.00 | 2.56 | 0.00 | 1.39 | -16.82 | 248.26 | 1.39 | 183.31 | 0.4050 | -862.0 | -772.7 | |
| 6.19 | 8.31 | 3.32 | 4.46 | -15.71 | 248.04 | 1.17 | 182.92 | 0.3869 | -942.9 | -622.4 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -15.22 | 247.47 | 0.60 | 181.55 | 0.3786 | -825.0 | -616.0 | |
| 0.00 | 0.62 | 0.00 | 0.34 | -17.18 | 247.44 | 0.58 | 181.35 | 0.4102 | -691.0 | -595.1 | |
| 0.00 | 0.80 | 0.00 | 0.43 | -17.15 | 247.26 | 0.39 | 180.91 | 0.4096 | -917.0 | -782.2 | |
| 0.00 | 0.53 | 0.00 | 0.28 | -15.87 | 247.13 | 0.26 | 180.65 | 0.3890 | -257.0 | -198.2 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -15.28 | 247.10 | 0.23 | 180.59 | 0.3795 | -794.0 | -591.9 | |
| 0.00 | 0.62 | 0.00 | 0.34 | -17.11 | 247.10 | 0.23 | 180.54 | 0.4090 | -835.0 | -709.4 | |
| 0.62 | 12.20 | 0.33 | 6.55 | -15.64 | 246.69 | -0.17 | 179.56 | 0.3853 | -936.4 | -703.6 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -14.63 | 246.66 | -0.20 | 179.46 | 0.3690 | -803.0 | -655.4 | |
| 0.00 | 2.92 | 0.00 | 1.57 | -15.96 | 246.38 | -0.49 | 178.79 | 0.3906 | -1003.0 | -867.5 | |
| 0.00 | 2.56 | 0.00 | 1.37 | -15.18 | 246.38 | -0.49 | 178.76 | 0.3780 | -779.0 | -709.6 | |
| 2.30 | 5.48 | 1.23 | 2.94 | -15.54 | 246.13 | -0.74 | 178.14 | 0.3839 | -1118.9 | -922.5 | |
| 1.77 | 11.23 | 0.95 | 5.99 | -15.18 | 246.10 | -0.77 | 178.04 | 0.3781 | -1084.6 | -909.9 | |
| 0.62 | 1.77 | 0.33 | 0.95 | -15.87 | 246.07 | -0.80 | 178.01 | 0.3892 | -934.1 | -821.9 | |
| 0.00 | 2.65 | 0.00 | 1.44 | -16.85 | 245.68 | -1.18 | 177.19 | 0.4052 | -600.0 | -568.0 | |
| 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. | |