| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.72 | 33.52 | 10.66 | 25.15 | -16.24 | 232.68 | -45.04 | 115.09 | 0.7510 | -224.7 | 3.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.73 | 0.00 | 0.46 | -15.60 | 243.80 | -33.92 | 120.23 | 0.6244 | 595.0 | 478.2 | |
| 0.00 | 1.18 | 0.00 | 0.80 | -17.68 | 239.59 | -38.13 | 120.40 | 0.6844 | 551.0 | 418.6 | |
| 1.27 | 3.36 | 0.89 | 2.35 | -14.13 | 236.10 | -41.63 | 113.82 | 0.7065 | 825.4 | 681.0 | |
| 0.00 | 1.00 | 0.00 | 0.70 | -14.36 | 235.92 | -41.81 | 114.05 | 0.7095 | 588.0 | 509.7 | |
| 0.73 | 2.18 | 0.51 | 1.53 | -14.37 | 235.66 | -42.06 | 113.94 | 0.7124 | 731.2 | 556.2 | |
| 0.00 | 0.45 | 0.00 | 0.32 | -14.18 | 235.70 | -42.02 | 113.71 | 0.7111 | 553.0 | 505.4 | |
| 0.00 | 1.73 | 0.00 | 1.23 | -15.00 | 235.21 | -42.51 | 114.56 | 0.7200 | 585.0 | 448.7 | |
| 0.00 | 1.27 | 0.00 | 0.92 | -15.93 | 234.31 | -43.41 | 115.36 | 0.7336 | 516.0 | 453.6 | |
| 0.00 | 1.00 | 0.00 | 0.73 | -15.49 | 234.08 | -43.64 | 114.69 | 0.7343 | -645.0 | -565.9 | |
| 0.00 | 2.45 | 0.00 | 1.82 | -16.07 | 233.21 | -44.51 | 115.05 | 0.7458 | -569.0 | -622.8 | |
| 0.00 | 1.00 | 0.00 | 0.74 | -16.18 | 233.05 | -44.67 | 115.11 | 0.7480 | -414.0 | -406.1 | |
| 0.00 | 1.09 | 0.00 | 0.81 | -15.86 | 232.92 | -44.81 | 114.65 | 0.7481 | -669.0 | -534.6 | |
| 11.72 | 15.26 | 9.26 | 12.06 | -17.26 | 230.22 | -47.51 | 115.27 | 0.7809 | -723.3 | -390.9 | |
| 0.00 | 0.82 | 0.00 | 0.68 | -15.88 | 227.14 | -50.59 | 112.47 | 0.8064 | -369.0 | -278.9 | |
| 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. | |