| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.25 | 24.18 | 2.24 | 16.44 | -20.60 | 158.45 | -34.41 | 129.37 | 0.6848 | 392.1 | 272.7 | |
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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 | 0.67 | -17.55 | 164.79 | -28.06 | 131.02 | 0.5967 | 753.0 | 633.9 | |
| 0.00 | 1.08 | 0.00 | 0.67 | -17.59 | 164.57 | -28.29 | 130.86 | 0.5994 | 702.0 | 532.0 | |
| 0.00 | 1.90 | 0.00 | 1.17 | -16.39 | 163.72 | -29.13 | 128.42 | 0.5984 | 759.0 | 585.9 | |
| 0.00 | 1.08 | 0.00 | 0.74 | -22.75 | 160.12 | -32.73 | 133.17 | 0.6860 | 697.0 | 602.8 | |
| 0.00 | 0.99 | 0.00 | 0.66 | -20.49 | 159.57 | -33.28 | 130.05 | 0.6738 | 710.0 | 526.5 | |
| 0.00 | 1.26 | 0.00 | 0.85 | -20.27 | 159.28 | -33.58 | 129.55 | 0.6751 | 560.0 | 416.4 | |
| 0.00 | 1.90 | 0.00 | 1.32 | -22.91 | 158.08 | -34.77 | 131.72 | 0.7060 | 566.0 | 477.0 | |
| 0.00 | 0.90 | 0.00 | 0.60 | -19.32 | 158.84 | -34.01 | 128.04 | 0.6725 | 524.0 | 458.8 | |
| 0.00 | 0.90 | 0.00 | 0.63 | -22.75 | 157.81 | -35.04 | 131.33 | 0.7074 | 259.0 | 251.0 | |
| 2.80 | 4.43 | 1.91 | 3.03 | -20.99 | 158.15 | -34.70 | 129.52 | 0.6914 | 789.1 | 559.8 | |
| 0.00 | 1.36 | 0.00 | 0.92 | -20.01 | 158.13 | -34.73 | 128.33 | 0.6846 | 627.0 | 465.3 | |
| 0.00 | 0.81 | 0.00 | 0.56 | -21.25 | 157.15 | -35.70 | 129.09 | 0.7029 | 404.0 | 292.6 | |
| 0.00 | 1.26 | 0.00 | 0.87 | -20.74 | 157.18 | -35.68 | 128.49 | 0.6991 | 607.0 | 513.6 | |
| 0.00 | 0.99 | 0.00 | 0.69 | -21.54 | 156.95 | -35.90 | 129.27 | 0.7069 | 465.0 | 302.5 | |
| 0.00 | 0.81 | 0.00 | 0.59 | -22.25 | 154.51 | -38.35 | 128.36 | 0.7346 | -569.0 | -595.8 | |
| 0.00 | 0.54 | 0.00 | 0.39 | -21.45 | 154.30 | -38.55 | 127.29 | 0.7314 | -518.0 | -488.7 | |
| 0.45 | 2.89 | 0.33 | 2.08 | -21.11 | 154.33 | -38.52 | 126.91 | 0.7290 | -678.2 | -643.1 | |
| 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. | |