| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.17 | 423.33 | 44.24 | 288.13 | -20.52 | 18.19 | -34.59 | 129.07 | 0.6871 | 932.9 | 284.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.79 | 2.63 | 0.51 | 1.71 | -18.81 | 20.51 | -32.27 | 128.82 | 0.6510 | 872.4 | 740.2 | |
| 0.00 | 1.14 | 0.00 | 0.74 | -18.65 | 20.36 | -32.42 | 128.50 | 0.6514 | 736.0 | 638.2 | |
| 0.00 | 2.01 | 0.00 | 1.33 | -19.45 | 19.76 | -33.02 | 129.00 | 0.6635 | 257.0 | 216.7 | |
| 0.00 | 0.26 | 0.00 | 0.17 | -18.95 | 19.73 | -33.06 | 128.36 | 0.6602 | 435.0 | 515.7 | |
| 0.00 | 1.31 | 0.00 | 0.91 | -22.56 | 18.61 | -34.17 | 131.80 | 0.6981 | -769.0 | -641.7 | |
| 2.19 | 405.81 | 1.47 | 276.22 | -20.31 | 19.14 | -33.65 | 129.56 | 0.6763 | 1184.8 | 294.2 | |
| 0.79 | 1.84 | 0.51 | 1.20 | -17.56 | 19.50 | -33.28 | 126.40 | 0.6523 | 779.8 | 701.5 | |
| 0.00 | 0.70 | 0.00 | 0.47 | -19.52 | 19.06 | -33.72 | 128.53 | 0.6712 | 666.0 | 605.5 | |
| 0.00 | 0.96 | 0.00 | 0.64 | -18.53 | 19.18 | -33.60 | 127.38 | 0.6627 | 599.0 | 508.6 | |
| 61.40 | -6.00 | 41.75 | -6.00 | -20.57 | 18.18 | -34.60 | 129.12 | 0.6876 | 1207.8 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.57 | -24.37 | 16.16 | -36.62 | 131.98 | 0.7332 | 513.0 | 395.6 | |
| 0.00 | 0.53 | 0.00 | 0.35 | -17.46 | 18.04 | -34.74 | 125.14 | 0.6671 | 512.0 | 429.8 | |
| 0.00 | 0.88 | 0.00 | 0.60 | -19.21 | 16.73 | -36.05 | 126.37 | 0.6925 | -409.0 | -467.7 | |
| 0.00 | 1.05 | 0.00 | 0.74 | -19.35 | 15.15 | -37.63 | 125.43 | 0.7094 | -584.0 | -548.4 | |
| 0.00 | 1.49 | 0.00 | 1.11 | -22.74 | 12.97 | -39.81 | 127.96 | 0.7512 | -519.0 | -412.1 | |
| 0.00 | 0.88 | 0.00 | 0.65 | -21.87 | 12.94 | -39.84 | 126.94 | 0.7462 | -497.0 | -460.3 | |
| 0.00 | 1.05 | 0.00 | 0.72 | -13.83 | 14.10 | -38.68 | 117.75 | 0.6880 | -552.0 | -402.8 | |
| 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. | |