| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 26.22 | 0.00 | 14.00 | -13.54 | 58.65 | -8.98 | 156.69 | 0.3743 | 24.2 | -92.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 4.91 | 0.00 | 2.59 | -13.08 | 62.48 | -5.15 | 165.20 | 0.3435 | 797.0 | 866.3 | |
| 0.00 | 1.14 | 0.00 | 0.60 | -14.17 | 62.33 | -5.30 | 165.59 | 0.3613 | 820.0 | 627.7 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -13.21 | 62.23 | -5.40 | 164.61 | 0.3466 | 786.0 | 569.4 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -13.69 | 61.91 | -5.72 | 164.13 | 0.3556 | 776.0 | 702.4 | |
| 0.00 | 3.42 | 0.00 | 1.80 | -12.22 | 60.53 | -7.10 | 159.08 | 0.3398 | -944.0 | -760.1 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -12.16 | 60.16 | -7.47 | 158.03 | 0.3411 | -738.0 | -617.3 | |
| 0.00 | 4.56 | 0.00 | 2.40 | -11.97 | 59.92 | -7.71 | 157.17 | 0.3398 | -1012.0 | -878.1 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -13.59 | 59.78 | -7.86 | 158.57 | 0.3652 | 924.0 | 689.4 | |
| 0.00 | 0.96 | 0.00 | 0.51 | -13.57 | 58.84 | -8.79 | 156.27 | 0.3707 | -720.0 | -600.5 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -14.85 | 57.22 | -10.41 | 154.01 | 0.4003 | 820.0 | 645.2 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -14.85 | 55.74 | -11.89 | 150.89 | 0.4112 | 811.0 | 686.0 | |
| 0.00 | 2.28 | 0.00 | 1.26 | -15.42 | 52.31 | -15.32 | 145.14 | 0.4473 | -599.0 | -665.5 | |
| 0.00 | 1.49 | 0.00 | 0.83 | -15.66 | 50.84 | -16.79 | 142.96 | 0.4637 | -733.0 | -545.2 | |
| 0.00 | 1.31 | 0.00 | 0.74 | -15.99 | 50.39 | -17.24 | 142.69 | 0.4720 | -649.0 | -559.5 | |
| 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. | |