| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.32 | 175.14 | 28.51 | 99.12 | -21.17 | 53.35 | 6.66 | 192.96 | 0.4866 | -65.3 | -202.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.55 | -16.17 | 61.38 | 14.69 | 212.06 | 0.4608 | 684.0 | 572.6 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -17.21 | 59.67 | 12.98 | 207.82 | 0.4614 | 731.0 | 534.3 | |
| 0.00 | 3.23 | 0.00 | 1.81 | -18.22 | 58.69 | 12.01 | 205.05 | 0.4686 | 528.0 | 586.9 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -16.68 | 58.53 | 11.84 | 206.25 | 0.4461 | 875.0 | 656.4 | |
| 0.00 | 1.71 | 0.00 | 0.98 | -21.98 | 56.53 | 9.84 | 198.19 | 0.5095 | 541.0 | 301.4 | |
| 15.54 | 35.93 | 8.87 | 20.52 | -21.35 | 56.12 | 9.43 | 197.90 | 0.4986 | 1030.7 | 451.2 | |
| 0.00 | 0.72 | 0.00 | 0.42 | -23.81 | 55.35 | 8.66 | 195.12 | 0.5306 | 703.0 | 522.5 | |
| 13.74 | 31.26 | 7.78 | 17.69 | -20.74 | 55.00 | 8.31 | 196.25 | 0.4848 | 1029.1 | 601.2 | |
| 1.35 | -8.00 | 0.76 | -8.00 | -21.08 | 54.85 | 8.16 | 195.78 | 0.4892 | 673.4 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.41 | -22.64 | 54.94 | 8.26 | 195.05 | 0.5123 | 570.0 | 497.6 | |
| 2.07 | 3.23 | 1.17 | 1.82 | -20.69 | 53.88 | 7.19 | 194.20 | 0.4796 | 841.3 | 701.8 | |
| 0.00 | 1.53 | 0.00 | 0.87 | -21.77 | 52.98 | 6.29 | 191.98 | 0.4927 | -716.0 | -573.7 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -19.24 | 52.85 | 6.16 | 192.94 | 0.4542 | -854.0 | -738.4 | |
| 0.00 | 1.98 | 0.00 | 1.13 | -22.36 | 52.88 | 6.19 | 191.52 | 0.5011 | -817.0 | -590.7 | |
| 0.00 | 1.26 | 0.00 | 0.70 | -19.24 | 52.59 | 5.90 | 192.42 | 0.4532 | -853.0 | -682.7 | |
| 0.00 | 1.08 | 0.00 | 0.60 | -20.29 | 52.56 | 5.87 | 191.86 | 0.4691 | -777.0 | -653.1 | |
| 0.00 | 4.04 | 0.00 | 2.29 | -21.56 | 52.35 | 5.66 | 190.89 | 0.4875 | -589.0 | -675.2 | |
| 0.00 | 2.07 | 0.00 | 1.17 | -21.87 | 52.20 | 5.51 | 190.48 | 0.4917 | -706.0 | -635.6 | |
| 0.00 | 1.17 | 0.00 | 0.65 | -20.32 | 52.11 | 5.42 | 190.95 | 0.4682 | -756.0 | -599.0 | |
| 2.52 | 47.25 | 1.42 | 26.60 | -21.24 | 52.01 | 5.32 | 190.38 | 0.4819 | -831.5 | -603.2 | |
| 0.00 | 2.25 | 0.00 | 1.26 | -20.59 | 51.99 | 5.30 | 190.60 | 0.4719 | -888.0 | -745.3 | |
| 0.00 | 1.17 | 0.00 | 0.66 | -21.90 | 52.00 | 5.31 | 190.11 | 0.4917 | -730.0 | -538.7 | |
| 11.77 | -20.00 | 6.63 | -20.00 | -21.03 | 51.58 | 4.89 | 189.63 | 0.4775 | -1067.4 | 999999 | |
| 1.35 | 2.43 | 0.76 | 1.37 | -21.34 | 50.97 | 4.28 | 188.35 | 0.4807 | -899.1 | -840.1 | |
| 0.00 | 6.29 | 0.00 | 3.57 | -21.96 | 50.82 | 4.14 | 187.88 | 0.4898 | -864.0 | -696.6 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -21.26 | 50.77 | 4.08 | 187.99 | 0.4792 | -902.0 | -751.3 | |
| 1.98 | 2.61 | 1.12 | 1.48 | -22.06 | 50.60 | 3.91 | 187.43 | 0.4908 | -890.0 | -749.4 | |
| 0.00 | 4.85 | 0.00 | 2.75 | -22.06 | 50.24 | 3.55 | 186.75 | 0.4901 | -1074.0 | -863.0 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -22.33 | 50.08 | 3.39 | 186.39 | 0.4940 | -684.0 | -561.8 | |
| 0.00 | 1.17 | 0.00 | 0.66 | -22.16 | 50.04 | 3.35 | 186.36 | 0.4913 | -937.0 | -742.4 | |
| 0.00 | 2.07 | 0.00 | 1.18 | -22.44 | 49.95 | 3.26 | 186.12 | 0.4954 | -647.0 | -518.2 | |
| 0.00 | 2.25 | 0.00 | 1.27 | -22.05 | 49.65 | 2.96 | 185.64 | 0.4891 | -738.0 | -748.8 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -22.82 | 49.60 | 2.91 | 185.38 | 0.5006 | -717.0 | -596.1 | |
| 0.00 | 0.72 | 0.00 | 0.41 | -23.30 | 48.88 | 2.19 | 183.99 | 0.5071 | -543.0 | -418.2 | |
| 0.00 | 1.44 | 0.00 | 0.83 | -24.22 | 48.66 | 1.98 | 183.48 | 0.5206 | -692.0 | -590.0 | |
| 0.00 | 0.99 | 0.00 | 0.57 | -24.01 | 48.59 | 1.91 | 183.38 | 0.5174 | -742.0 | -686.8 | |
| 0.00 | 2.34 | 0.00 | 1.32 | -22.15 | 46.87 | 0.18 | 180.34 | 0.4883 | -866.0 | -705.7 | |
| 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. | |