| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.53 | 0.00 | 9.66 | 7.95 | 261.88 | -14.75 | 105.21 | 0.2809 | 615.8 | 487.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.00 | 0.00 | 0.50 | 3.43 | 280.45 | 3.82 | 273.27 | 0.0669 | -789.0 | -593.8 | |
| 0.00 | 1.82 | 0.00 | 0.90 | 6.31 | 278.04 | 1.42 | 335.49 | 0.0595 | -764.0 | -495.3 | |
| 0.00 | 1.64 | 0.00 | 0.82 | 9.35 | 269.86 | -6.77 | 47.34 | 0.1589 | 1140.0 | 854.8 | |
| 0.00 | 0.82 | 0.00 | 0.42 | 12.22 | 266.83 | -9.80 | 46.59 | 0.2299 | 708.0 | 480.7 | |
| 0.00 | 1.64 | 0.00 | 0.83 | 8.61 | 265.22 | -11.41 | 64.08 | 0.2185 | 955.0 | 654.9 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 3.26 | 264.58 | -12.05 | 89.45 | 0.2094 | 874.0 | 674.0 | |
| 0.00 | 0.73 | 0.00 | 0.37 | 9.62 | 261.73 | -14.90 | 65.94 | 0.2789 | 899.0 | 817.0 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 9.03 | 261.69 | -14.94 | 67.95 | 0.2760 | 1072.0 | 838.4 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 9.09 | 261.52 | -15.10 | 67.95 | 0.2788 | 1037.0 | 846.5 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 9.00 | 261.37 | -15.26 | 68.46 | 0.2807 | 851.0 | 743.2 | |
| 0.00 | 1.54 | 0.00 | 0.85 | 8.66 | 251.30 | -25.32 | 76.67 | 0.4364 | 695.0 | 560.3 | |
| 0.00 | 1.54 | 0.00 | 0.85 | 7.74 | 251.02 | -25.60 | 78.87 | 0.4382 | 724.0 | 555.9 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 8.15 | 250.45 | -26.18 | 78.14 | 0.4481 | 602.0 | 435.3 | |
| 0.00 | 1.36 | 0.00 | 0.75 | 7.17 | 250.41 | -26.22 | 80.33 | 0.4465 | 617.0 | 539.5 | |
| 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. | |