| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.86 | 26.67 | 3.46 | 15.82 | 20.21 | 109.62 | 31.08 | 298.20 | 0.5517 | 306.1 | 60.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.66 | 0.00 | 1.00 | 20.00 | 111.18 | 32.64 | 296.95 | 0.5707 | -649.0 | -600.1 | |
| 0.00 | 1.84 | 0.00 | 1.11 | 20.96 | 111.33 | 32.79 | 298.43 | 0.5773 | -607.0 | -445.8 | |
| 0.00 | 1.05 | 0.00 | 0.63 | 20.42 | 110.93 | 32.39 | 297.78 | 0.5696 | -704.0 | -627.3 | |
| 2.10 | 6.56 | 1.26 | 3.94 | 20.40 | 110.74 | 32.20 | 297.85 | 0.5671 | -934.6 | -800.8 | |
| 0.00 | 2.45 | 0.00 | 1.45 | 19.82 | 109.37 | 30.83 | 297.68 | 0.5466 | 864.0 | 661.1 | |
| 0.00 | 1.22 | 0.00 | 0.72 | 20.16 | 109.37 | 30.83 | 298.26 | 0.5484 | 545.0 | 468.4 | |
| 0.00 | 1.31 | 0.00 | 0.77 | 20.14 | 109.18 | 30.64 | 298.35 | 0.5459 | 791.0 | 671.7 | |
| 0.00 | 1.92 | 0.00 | 1.13 | 20.21 | 109.01 | 30.47 | 298.57 | 0.5440 | 790.0 | 678.5 | |
| 1.66 | 1.92 | 0.97 | 1.13 | 19.54 | 108.69 | 30.15 | 297.63 | 0.5363 | 764.1 | 500.3 | |
| 2.10 | 2.54 | 1.23 | 1.49 | 19.88 | 108.72 | 30.18 | 298.20 | 0.5385 | 836.0 | 752.4 | |
| 0.00 | 1.22 | 0.00 | 0.72 | 19.62 | 108.48 | 29.94 | 297.88 | 0.5340 | 922.0 | 821.5 | |
| 0.00 | 0.79 | 0.00 | 0.46 | 22.14 | 108.37 | 29.83 | 302.28 | 0.5471 | 647.0 | 464.9 | |
| 0.00 | 1.14 | 0.00 | 0.67 | 21.67 | 107.86 | 29.32 | 301.85 | 0.5378 | 667.0 | 597.2 | |
| 0.00 | 1.05 | 0.00 | 0.60 | 18.35 | 105.97 | 27.43 | 297.26 | 0.4938 | 568.0 | 550.1 | |
| 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. | |