| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.62 | 224.70 | 45.98 | 182.49 | -19.53 | 107.35 | -45.75 | 121.56 | 0.7945 | 751.4 | 364.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.54 | 0.00 | 0.42 | -19.88 | 109.56 | -43.54 | 123.17 | 0.7762 | -486.0 | -397.5 | |
| 0.00 | 0.98 | 0.00 | 0.82 | -22.78 | 107.71 | -45.39 | 125.36 | 0.8071 | 590.0 | 482.7 | |
| 0.80 | 5.98 | 0.67 | 5.00 | -22.62 | 107.59 | -45.51 | 125.12 | 0.8073 | 652.2 | 612.6 | |
| 0.00 | 1.52 | 0.00 | 1.22 | -19.86 | 108.31 | -44.79 | 122.45 | 0.7875 | 722.0 | 536.2 | |
| 0.00 | 0.89 | 0.00 | 0.75 | -22.22 | 107.11 | -46.00 | 124.42 | 0.8094 | 477.0 | 424.7 | |
| 0.00 | 0.71 | 0.00 | 0.58 | -19.67 | 107.88 | -45.22 | 122.00 | 0.7904 | 550.0 | 479.9 | |
| 0.80 | 35.73 | 0.66 | 29.40 | -20.76 | 107.42 | -45.68 | 122.98 | 0.7997 | 710.6 | 378.4 | |
| 20.99 | 88.24 | 16.65 | 69.78 | -18.68 | 108.14 | -44.96 | 121.01 | 0.7833 | 956.3 | 506.0 | |
| 9.29 | -7.00 | 7.66 | -7.00 | -20.65 | 107.14 | -45.96 | 122.71 | 0.8017 | 747.8 | 999999 | |
| 0.00 | 0.71 | 0.00 | 0.57 | -18.63 | 107.56 | -45.54 | 120.65 | 0.7884 | 245.0 | 177.0 | |
| 0.27 | 85.65 | 0.22 | 70.63 | -19.44 | 107.09 | -46.01 | 121.32 | 0.7965 | 755.3 | 232.1 | |
| 20.63 | -11.00 | 16.98 | -11.00 | -19.81 | 106.81 | -46.29 | 121.59 | 0.8006 | 880.8 | 999999 | |
| 3.57 | -11.00 | 2.92 | -11.00 | -19.08 | 106.71 | -46.39 | 120.72 | 0.7982 | 734.5 | 999999 | |
| 0.27 | -11.00 | 0.22 | -11.00 | -18.89 | 106.64 | -46.46 | 120.46 | 0.7979 | 560.3 | 999999 | |
| 0.00 | 0.71 | 0.00 | 0.62 | -21.76 | 105.15 | -47.96 | 122.90 | 0.8237 | 348.0 | 352.1 | |
| 0.00 | 1.79 | 0.00 | 1.57 | -18.04 | 102.77 | -50.34 | 117.68 | 0.8286 | -520.0 | -517.5 | |
| 0.00 | 1.25 | 0.00 | 1.13 | -18.10 | 101.52 | -51.58 | 117.21 | 0.8394 | -374.0 | -348.8 | |
| 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. | |