| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.50 | 426.15 | 35.79 | 232.86 | 17.74 | 166.60 | 10.32 | 336.17 | 0.4234 | -664.3 | -297.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.24 | 387.44 | 33.50 | 211.98 | 17.74 | 167.06 | 10.78 | 335.15 | 0.4258 | -1391.3 | -399.1 | |
| 0.00 | 0.98 | 0.00 | 0.53 | 18.56 | 165.40 | 9.13 | 339.33 | 0.4276 | -752.0 | -619.5 | |
| 0.00 | 0.98 | 0.00 | 0.53 | 16.66 | 164.79 | 8.52 | 338.91 | 0.3960 | 647.0 | 446.0 | |
| 0.00 | 1.24 | 0.00 | 0.67 | 17.95 | 163.29 | 7.01 | 343.38 | 0.4077 | 961.0 | 775.2 | |
| 0.00 | 2.13 | 0.00 | 1.15 | 17.30 | 163.23 | 6.95 | 343.01 | 0.3974 | 775.0 | 646.8 | |
| 0.00 | 0.89 | 0.00 | 0.48 | 18.70 | 163.13 | 6.85 | 344.26 | 0.4185 | 639.0 | 566.0 | |
| 0.00 | 1.24 | 0.00 | 0.68 | 18.51 | 163.12 | 6.84 | 344.15 | 0.4154 | 714.0 | 633.5 | |
| 0.00 | 2.49 | 0.00 | 1.35 | 17.91 | 162.91 | 6.63 | 344.21 | 0.4054 | 1008.0 | 858.9 | |
| 0.00 | 1.51 | 0.00 | 0.82 | 18.31 | 162.92 | 6.64 | 344.45 | 0.4115 | 806.0 | 644.6 | |
| 0.00 | 1.42 | 0.00 | 0.77 | 17.98 | 162.59 | 6.31 | 344.97 | 0.4050 | 962.0 | 825.6 | |
| 0.00 | 1.86 | 0.00 | 1.02 | 19.26 | 162.61 | 6.33 | 345.76 | 0.4248 | 773.0 | 635.2 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 17.91 | 162.33 | 6.05 | 345.51 | 0.4029 | 897.0 | 791.9 | |
| 0.00 | 0.89 | 0.00 | 0.48 | 18.96 | 162.34 | 6.06 | 346.16 | 0.4192 | 777.0 | 643.8 | |
| 0.00 | 1.60 | 0.00 | 0.86 | 18.07 | 162.08 | 5.81 | 346.19 | 0.4045 | 636.0 | 511.4 | |
| 0.00 | 0.89 | 0.00 | 0.48 | 17.41 | 161.97 | 5.69 | 346.04 | 0.3938 | 674.0 | 544.7 | |
| 0.00 | 9.32 | 0.00 | 5.01 | 17.31 | 161.36 | 5.08 | 347.42 | 0.3900 | 1049.0 | 775.2 | |
| 1.24 | 2.66 | 0.67 | 1.43 | 17.80 | 160.42 | 4.14 | 349.92 | 0.3947 | 861.1 | 643.5 | |
| 3.02 | 7.46 | 1.62 | 4.00 | 17.34 | 160.25 | 3.98 | 350.11 | 0.3869 | 1064.1 | 784.7 | |
| 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. | |