| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.65 | 161.05 | 17.33 | 88.33 | -20.81 | 18.79 | -15.70 | 144.09 | 0.4323 | 823.8 | 423.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.75 | 129.22 | 16.28 | 70.62 | -20.65 | 19.22 | -15.27 | 144.52 | 0.4263 | 1232.3 | 455.6 | |
| 1.90 | 3.62 | 1.05 | 1.99 | -21.04 | 18.57 | -15.92 | 143.98 | 0.4371 | 831.7 | 725.8 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -21.40 | 18.43 | -16.06 | 144.26 | 0.4428 | 617.0 | 499.7 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -21.14 | 18.32 | -16.17 | 143.71 | 0.4406 | 736.0 | 573.0 | |
| 0.00 | 0.81 | 0.00 | 0.45 | -21.99 | 18.09 | -16.40 | 144.53 | 0.4530 | 678.0 | 466.8 | |
| 0.00 | 1.99 | 0.00 | 1.10 | -21.59 | 18.10 | -16.39 | 144.00 | 0.4482 | 847.0 | 664.1 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -21.82 | 17.73 | -16.76 | 143.73 | 0.4543 | 626.0 | 483.6 | |
| 0.00 | 8.32 | 0.00 | 4.61 | -21.37 | 17.72 | -16.77 | 143.06 | 0.4490 | 760.0 | 676.4 | |
| 0.00 | 6.33 | 0.00 | 3.49 | -20.49 | 17.78 | -16.70 | 141.87 | 0.4379 | 102.0 | 163.7 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -21.79 | 17.53 | -16.96 | 143.37 | 0.4558 | 564.0 | 485.9 | |
| 0.00 | 2.17 | 0.00 | 1.21 | -22.28 | 17.30 | -17.19 | 143.69 | 0.4638 | 597.0 | 417.8 | |
| 0.00 | 1.45 | 0.00 | 0.84 | -23.23 | 12.78 | -21.71 | 138.76 | 0.5176 | -798.0 | -670.7 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -22.86 | 12.81 | -21.68 | 138.28 | 0.5136 | -779.0 | -579.4 | |
| 0.00 | 2.17 | 0.00 | 1.25 | -22.30 | 12.08 | -22.41 | 136.59 | 0.5152 | -722.0 | -615.5 | |
| 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. | |