| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.78 | 146.74 | 34.57 | 193.17 | -13.60 | 230.28 | -67.93 | 103.32 | 0.9225 | 336.4 | 146.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.16 | 0.00 | 1.12 | -10.13 | 239.24 | -58.97 | 99.83 | 0.8581 | 561.0 | 474.9 | |
| 0.00 | 0.72 | 0.00 | 0.71 | -10.16 | 238.07 | -60.14 | 99.82 | 0.8683 | 325.0 | 296.6 | |
| 16.30 | 102.57 | 17.80 | 112.62 | -11.67 | 235.10 | -63.11 | 101.42 | 0.8929 | 804.6 | 265.0 | |
| 2.33 | -3.00 | 2.59 | -3.00 | -11.49 | 234.48 | -63.73 | 101.18 | 0.8976 | 361.9 | 999999 | |
| 1.70 | -3.00 | 1.89 | -3.00 | -11.21 | 234.52 | -63.69 | 100.88 | 0.8972 | 404.4 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.47 | -19.53 | 224.52 | -73.69 | 109.40 | 0.9602 | -81.0 | -90.3 | |
| 0.00 | 0.27 | 0.00 | 0.43 | -15.05 | 225.97 | -72.24 | 104.75 | 0.9524 | -404.0 | -384.0 | |
| 0.00 | 1.16 | 0.00 | 1.86 | -14.83 | 225.95 | -72.26 | 104.52 | 0.9524 | -341.0 | -275.8 | |
| 0.00 | 0.81 | 0.00 | 1.28 | -14.43 | 226.17 | -72.04 | 104.11 | 0.9513 | 88.0 | 124.7 | |
| 0.00 | 0.99 | 0.00 | 1.68 | -15.68 | 224.86 | -73.35 | 105.38 | 0.9580 | -231.0 | -184.2 | |
| 6.45 | 33.05 | 12.29 | 63.18 | -17.02 | 222.95 | -75.26 | 106.74 | 0.9668 | 129.8 | 34.0 | |
| 0.00 | 0.63 | 0.00 | 1.09 | -15.53 | 224.44 | -73.77 | 105.22 | 0.9600 | -124.0 | -61.3 | |
| 0.00 | 0.81 | 0.00 | 1.38 | -15.20 | 224.75 | -73.46 | 104.88 | 0.9584 | -389.0 | -425.1 | |
| 0.00 | 0.90 | 0.00 | 1.56 | -15.34 | 224.40 | -73.81 | 105.02 | 0.9602 | -193.0 | -171.7 | |
| 0.00 | 1.16 | 0.00 | 1.92 | -13.73 | 225.37 | -72.84 | 103.36 | 0.9553 | -147.0 | -197.7 | |
| 0.00 | 1.25 | 0.00 | 1.97 | -11.21 | 226.33 | -71.88 | 100.72 | 0.9502 | -281.0 | -277.4 | |
| 0.00 | 0.99 | 0.00 | 1.90 | -14.12 | 222.82 | -75.39 | 103.74 | 0.9672 | -398.0 | -279.4 | |
| 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. | |