| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13 | 166 | 7 | 103 | -27.55 | 292.76 | -16.18 | 154.85 | 0.5834 | 799.5 | 690.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 5 | 0 | 3 | -26.83 | 295.68 | -13.25 | 158.37 | 0.5573 | 841.0 | 693.3 | |
| 0 | 4 | 0 | 2 | -29.12 | 295.39 | -13.54 | 159.58 | 0.5888 | 585.0 | 592.4 | |
| 0 | 4 | 0 | 2 | -28.85 | 295.02 | -13.92 | 158.89 | 0.5871 | 707.0 | 752.1 | |
| 0 | 4 | 0 | 3 | -27.11 | 295.20 | -13.73 | 157.89 | 0.5635 | 723.0 | 671.4 | |
| 0 | 5 | 0 | 3 | -28.12 | 294.85 | -14.09 | 158.13 | 0.5786 | 699.0 | 587.6 | |
| 0 | 3 | 0 | 2 | -26.44 | 295.02 | -13.92 | 157.11 | 0.5557 | 787.0 | 622.2 | |
| 0 | 5 | 0 | 3 | -26.41 | 294.14 | -14.80 | 155.81 | 0.5605 | 836.0 | 828.1 | |
| 0 | 23 | 0 | 14 | -26.33 | 293.66 | -15.28 | 155.06 | 0.5624 | 1143.0 | 812.3 | |
| 0 | 5 | 0 | 3 | -25.39 | 293.69 | -15.24 | 154.31 | 0.5501 | 679.0 | 595.9 | |
| 9 | 27 | 5 | 17 | -29.64 | 292.52 | -16.42 | 156.18 | 0.6105 | 942.5 | 585.0 | |
| 0 | 6 | 0 | 4 | -26.90 | 292.50 | -16.44 | 153.94 | 0.5767 | 812.0 | 680.7 | |
| 0 | 8 | 0 | 5 | -26.22 | 292.47 | -16.47 | 153.31 | 0.5685 | 799.0 | 753.5 | |
| 4 | 8 | 2 | 5 | -29.14 | 291.96 | -16.98 | 155.08 | 0.6077 | 550.4 | 443.2 | |
| 0 | 4 | 0 | 2 | -28.46 | 291.71 | -17.23 | 154.21 | 0.6008 | 688.0 | 483.9 | |
| 0 | 31 | 0 | 19 | -26.64 | 291.73 | -17.21 | 152.68 | 0.5785 | 902.0 | 893.4 | |
| 0 | 6 | 0 | 4 | -27.28 | 291.54 | -17.40 | 152.99 | 0.5875 | 743.0 | 673.0 | |
| 0 | 4 | 0 | 3 | -29.26 | 291.15 | -17.79 | 154.16 | 0.6138 | 695.0 | 542.0 | |
| 0 | 4 | 0 | 3 | -28.61 | 291.22 | -17.72 | 153.72 | 0.6056 | 575.0 | 454.7 | |
| 0 | 2 | 0 | 1 | -27.88 | 291.16 | -17.77 | 153.03 | 0.5972 | 454.0 | 591.5 | |
| 0 | 8 | 0 | 5 | -27.38 | 291.20 | -17.74 | 152.64 | 0.5909 | 639.0 | 553.2 | |
| 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. | |