| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.82 | 276.06 | 36.65 | 190.35 | -21.62 | 331.84 | 35.63 | 231.20 | 0.6972 | -366.5 | -289.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.30 | 4.95 | 0.97 | 3.69 | -19.73 | 338.32 | 42.11 | 237.73 | 0.7488 | 431.7 | 471.0 | |
| 1.13 | 1.74 | 0.84 | 1.29 | -19.43 | 338.13 | 41.92 | 237.99 | 0.7454 | 448.5 | 401.9 | |
| 0.00 | 1.91 | 0.00 | 1.41 | -19.38 | 337.82 | 41.61 | 237.87 | 0.7420 | 613.0 | 498.5 | |
| 0.00 | 1.82 | 0.00 | 1.34 | -19.04 | 337.67 | 41.46 | 238.20 | 0.7388 | 658.0 | 575.4 | |
| 0.00 | 1.56 | 0.00 | 1.14 | -19.05 | 337.30 | 41.09 | 237.97 | 0.7351 | 709.0 | 528.1 | |
| 8.43 | 20.59 | 6.09 | 14.86 | -18.80 | 336.93 | 40.72 | 238.06 | 0.7301 | 863.7 | 662.0 | |
| 2.61 | -6.00 | 1.87 | -6.00 | -18.50 | 336.80 | 40.59 | 238.35 | 0.7271 | 831.6 | 999999 | |
| 0.00 | 1.56 | 0.00 | 1.14 | -19.46 | 337.04 | 40.83 | 237.33 | 0.7348 | 440.0 | 400.1 | |
| 0.00 | 0.96 | 0.00 | 0.69 | -19.51 | 336.81 | 40.60 | 237.12 | 0.7327 | 601.0 | 478.6 | |
| 0.00 | 0.96 | 0.00 | 0.68 | -19.17 | 336.04 | 39.83 | 237.08 | 0.7231 | 775.0 | 687.0 | |
| 0.00 | 1.04 | 0.00 | 0.73 | -18.84 | 335.33 | 39.12 | 237.05 | 0.7140 | 723.0 | 592.9 | |
| 0.00 | 0.78 | 0.00 | 0.55 | -21.20 | 333.79 | 37.58 | 233.15 | 0.7128 | -479.0 | -459.6 | |
| 0.00 | 1.48 | 0.00 | 1.04 | -22.40 | 333.22 | 37.01 | 231.33 | 0.7152 | -327.0 | -277.6 | |
| 0.00 | 0.61 | 0.00 | 0.42 | -21.64 | 332.79 | 36.58 | 231.93 | 0.7060 | -440.0 | -449.1 | |
| 5.30 | 236.10 | 3.63 | 161.37 | -21.60 | 331.47 | 35.26 | 231.02 | 0.6928 | -862.4 | -397.8 | |
| 1.22 | -15.00 | 0.83 | -15.00 | -21.96 | 331.34 | 35.13 | 230.49 | 0.6940 | -615.8 | 999999 | |
| 32.83 | -15.00 | 22.42 | -15.00 | -22.13 | 330.83 | 34.62 | 229.90 | 0.6904 | -1085.7 | 999999 | |
| 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. | |