| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.37 | 0.00 | 11.47 | 18.85 | 359.63 | -8.53 | 33.05 | 0.2526 | -641.9 | -628.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.51 | 21.00 | 1.84 | -6.32 | 23.01 | 0.2640 | -841.0 | -677.3 | |
| 0.00 | 5.02 | 0.00 | 2.55 | 17.78 | 1.86 | -6.29 | 29.16 | 0.2150 | -925.0 | -806.2 | |
| 0.00 | 1.53 | 0.00 | 0.78 | 20.15 | 1.19 | -6.96 | 26.57 | 0.2557 | -840.0 | -594.5 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 20.12 | 1.00 | -7.16 | 27.26 | 0.2566 | -849.0 | -777.9 | |
| 0.00 | 1.61 | 0.00 | 0.82 | 17.70 | 0.65 | -7.50 | 33.79 | 0.2247 | -827.0 | -764.3 | |
| 0.00 | 1.79 | 0.00 | 0.92 | 19.76 | 0.17 | -7.99 | 30.57 | 0.2582 | -994.0 | -855.8 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 19.27 | 0.19 | -7.96 | 31.56 | 0.2509 | -886.0 | -674.8 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 19.08 | 0.07 | -8.08 | 32.36 | 0.2493 | -927.0 | -772.0 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 17.81 | 0.04 | -8.12 | 35.57 | 0.2322 | -904.0 | -724.3 | |
| 0.00 | 1.53 | 0.00 | 0.78 | 17.38 | 0.02 | -8.13 | 36.77 | 0.2265 | -790.0 | -658.2 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 17.81 | 359.81 | -8.34 | 36.31 | 0.2343 | -770.0 | -598.2 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 18.61 | 359.67 | -8.48 | 34.71 | 0.2465 | -865.0 | -718.1 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 19.19 | 359.35 | -8.80 | 34.30 | 0.2575 | -679.0 | -551.9 | |
| 0.00 | 0.63 | 0.00 | 0.35 | 22.90 | 347.26 | -20.89 | 49.50 | 0.4338 | 669.0 | 580.4 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 19.82 | 346.58 | -21.58 | 56.46 | 0.4168 | 800.0 | 578.6 | |
| 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. | |