| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.22 | 434.49 | 36.15 | 230.12 | 16.67 | 110.16 | 13.66 | 320.37 | 0.3563 | -1022.7 | -377.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.82 | 420.38 | 34.88 | 222.73 | 16.62 | 110.35 | 13.85 | 319.85 | 0.3574 | -1607.3 | -418.5 | |
| 0.26 | -1.00 | 0.14 | -1.00 | 17.08 | 110.32 | 13.82 | 320.76 | 0.3627 | -922.3 | 999999 | |
| 2.14 | -1.00 | 1.13 | -1.00 | 16.96 | 109.74 | 13.24 | 321.72 | 0.3553 | -1082.2 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 17.99 | 107.46 | 10.97 | 328.45 | 0.3474 | 684.0 | 514.0 | |
| 0.00 | 1.88 | 0.00 | 0.99 | 17.62 | 107.06 | 10.57 | 328.79 | 0.3388 | 789.0 | 653.7 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 18.14 | 106.71 | 10.22 | 330.44 | 0.3433 | 874.0 | 679.2 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 16.94 | 105.36 | 8.86 | 332.00 | 0.3153 | 854.0 | 773.7 | |
| 0.00 | 2.22 | 0.00 | 1.16 | 17.07 | 105.21 | 8.71 | 332.59 | 0.3160 | 1140.0 | 867.8 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 18.24 | 104.51 | 8.02 | 336.10 | 0.3284 | 702.0 | 542.8 | |
| 0.00 | 1.97 | 0.00 | 1.03 | 17.47 | 104.38 | 7.89 | 335.40 | 0.3159 | 754.0 | 463.0 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 18.37 | 104.05 | 7.55 | 337.49 | 0.3272 | 792.0 | 580.1 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 19.09 | 103.70 | 7.21 | 339.24 | 0.3360 | 773.0 | 594.9 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 15.30 | 102.68 | 6.19 | 337.35 | 0.2714 | 965.0 | 735.7 | |
| 0.00 | 0.60 | 0.00 | 0.31 | 15.66 | 102.36 | 5.86 | 338.95 | 0.2751 | 766.0 | 606.7 | |
| 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. | |