| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.24 | 0.00 | 11.36 | -19.24 | 159.68 | -11.16 | 157.09 | 0.4684 | 657.3 | 503.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.08 | 0.00 | 0.59 | -17.25 | 164.70 | -6.13 | 165.64 | 0.4130 | 802.0 | 706.2 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -19.27 | 163.72 | -7.11 | 164.80 | 0.4477 | 632.0 | 537.7 | |
| 0.00 | 1.08 | 0.00 | 0.60 | -19.39 | 162.12 | -8.71 | 161.69 | 0.4567 | 674.0 | 574.8 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -17.51 | 160.57 | -10.26 | 157.06 | 0.4378 | 936.0 | 737.5 | |
| 0.00 | 1.72 | 0.00 | 0.96 | -19.80 | 160.03 | -10.80 | 158.05 | 0.4737 | 921.0 | 719.6 | |
| 0.00 | 1.72 | 0.00 | 0.97 | -20.32 | 159.83 | -11.00 | 158.11 | 0.4821 | 806.0 | 571.2 | |
| 0.00 | 1.99 | 0.00 | 1.10 | -17.50 | 159.83 | -11.01 | 155.57 | 0.4422 | 930.0 | 754.9 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -20.49 | 159.59 | -11.25 | 157.82 | 0.4860 | 792.0 | 662.3 | |
| 0.00 | 1.90 | 0.00 | 1.08 | -20.87 | 159.49 | -11.34 | 157.96 | 0.4918 | 756.0 | 596.2 | |
| 0.00 | 0.99 | 0.00 | 0.57 | -21.66 | 159.43 | -11.41 | 158.48 | 0.5032 | 600.0 | 436.5 | |
| 0.00 | 1.90 | 0.00 | 1.05 | -17.33 | 159.61 | -11.23 | 154.99 | 0.4413 | 929.0 | 789.5 | |
| 0.00 | 1.63 | 0.00 | 0.90 | -17.07 | 159.53 | -11.31 | 154.56 | 0.4382 | 970.0 | 743.2 | |
| 0.00 | 0.63 | 0.00 | 0.35 | -17.47 | 159.27 | -11.56 | 154.48 | 0.4455 | 126.0 | 141.6 | |
| 0.00 | 2.35 | 0.00 | 1.38 | -21.86 | 154.55 | -16.29 | 150.88 | 0.5370 | -672.0 | -546.3 | |
| 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. | |