| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.67 | 46.33 | 10.12 | 23.92 | -23.28 | 180.44 | 2.83 | 189.64 | 0.2834 | -238.4 | -497.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.91 | 13.80 | 6.11 | 7.09 | -21.72 | 182.71 | 5.10 | 198.23 | 0.2654 | 1088.8 | 844.4 | |
| 0.00 | 1.55 | 0.00 | 0.80 | -22.01 | 181.73 | 4.12 | 194.60 | 0.2653 | 1138.0 | 951.6 | |
| 6.38 | 8.63 | 3.30 | 4.46 | -23.62 | 179.99 | 2.38 | 187.68 | 0.2864 | -942.4 | -790.5 | |
| 0.00 | 3.80 | 0.00 | 1.96 | -23.93 | 179.77 | 2.16 | 186.83 | 0.2911 | -900.0 | -780.5 | |
| 0.00 | 1.73 | 0.00 | 0.89 | -22.88 | 179.75 | 2.14 | 187.27 | 0.2735 | -768.0 | -514.0 | |
| 0.00 | 0.95 | 0.00 | 0.49 | -23.44 | 179.73 | 2.12 | 186.93 | 0.2827 | -1019.0 | -857.8 | |
| 0.00 | 1.55 | 0.00 | 0.80 | -24.09 | 179.61 | 2.00 | 186.26 | 0.2934 | -673.0 | -618.2 | |
| 0.00 | 1.21 | 0.00 | 0.62 | -22.98 | 179.56 | 1.95 | 186.58 | 0.2747 | -837.0 | -649.4 | |
| 0.00 | 5.26 | 0.00 | 2.74 | -24.93 | 179.29 | 1.69 | 185.01 | 0.3068 | -742.0 | -653.1 | |
| 0.00 | 1.98 | 0.00 | 1.03 | -24.71 | 179.06 | 1.45 | 184.39 | 0.3029 | -902.0 | -711.3 | |
| 1.38 | 1.47 | 0.71 | 0.76 | -24.06 | 178.70 | 1.09 | 183.43 | 0.2916 | -866.1 | -913.0 | |
| 0.00 | 0.95 | 0.00 | 0.49 | -23.85 | 178.27 | 0.67 | 182.13 | 0.2877 | -890.0 | -711.3 | |
| 0.00 | 0.95 | 0.00 | 0.49 | -24.44 | 178.28 | 0.67 | 182.05 | 0.2975 | -925.0 | -732.7 | |
| 0.00 | 1.21 | 0.00 | 0.63 | -24.44 | 178.05 | 0.44 | 181.35 | 0.2974 | -836.0 | -728.5 | |
| 0.00 | 1.29 | 0.00 | 0.67 | -24.62 | 177.26 | -0.34 | 178.96 | 0.3005 | -847.0 | -734.3 | |
| 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. | |