| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 95 | 589 | 63 | 398 | 19.07 | 31.72 | -40.74 | 65.21 | 0.6811 | 57.2 | 47.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 2 | 18.05 | 38.61 | -33.85 | 63.62 | 0.5933 | 573.0 | 381.5 | |
| 0 | 4 | 0 | 2 | 17.58 | 37.96 | -34.50 | 64.72 | 0.5994 | 451.0 | 346.0 | |
| 22 | 274 | 14 | 180 | 19.67 | 35.01 | -37.45 | 63.00 | 0.6449 | 1460.4 | 489.7 | |
| -3 | -3 | -3 | -3 | 19.37 | 34.72 | -37.74 | 63.58 | 0.6470 | 999999 | 999999 | |
| 12 | -3 | 8 | -3 | 20.55 | 32.86 | -39.60 | 62.73 | 0.6738 | 1000.9 | 999999 | |
| 0 | 16 | 0 | 11 | 17.93 | 32.64 | -39.82 | 66.56 | 0.6663 | -829.0 | -628.1 | |
| 0 | 6 | 0 | 4 | 19.64 | 31.98 | -40.48 | 64.38 | 0.6803 | 403.0 | 184.1 | |
| 0 | 9 | 0 | 6 | 19.19 | 31.00 | -41.45 | 65.40 | 0.6900 | 349.0 | 198.6 | |
| 7 | 25 | 5 | 17 | 17.83 | 31.02 | -41.44 | 67.31 | 0.6852 | -908.7 | -739.2 | |
| 0 | 4 | 0 | 3 | 19.82 | 30.01 | -42.45 | 64.91 | 0.7034 | -436.0 | -363.7 | |
| 8 | 230 | 5 | 161 | 18.04 | 30.11 | -42.34 | 67.32 | 0.6964 | -1315.9 | -290.9 | |
| 16 | -11 | 11 | -11 | 18.15 | 29.63 | -42.83 | 67.34 | 0.7024 | -1221.7 | 999999 | |
| 15 | -11 | 10 | -11 | 18.71 | 29.34 | -43.12 | 66.66 | 0.7074 | -810.8 | 999999 | |
| 15 | -11 | 10 | -11 | 18.79 | 28.21 | -44.25 | 66.92 | 0.7204 | 808.9 | 999999 | |
| 0 | 4 | 0 | 2 | 17.81 | 28.35 | -44.11 | 68.21 | 0.7159 | -702.0 | -381.9 | |
| 0 | 13 | 0 | 10 | 17.32 | 27.45 | -45.01 | 69.14 | 0.7248 | -679.0 | -451.7 | |
| 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. | |