| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.84 | 41.18 | 8.03 | 25.14 | 16.24 | 27.86 | 29.31 | 306.54 | 0.5861 | -66.5 | 71.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.59 | 12.41 | 5.41 | 7.82 | 15.94 | 31.03 | 32.48 | 303.25 | 0.6198 | -894.2 | -563.1 | |
| 2.89 | 4.68 | 1.81 | 2.92 | 16.06 | 30.33 | 31.78 | 303.98 | 0.6126 | -839.4 | -625.0 | |
| 0.00 | 1.19 | 0.00 | 0.74 | 16.05 | 29.93 | 31.38 | 304.28 | 0.6079 | -695.0 | -587.4 | |
| 0.00 | 1.70 | 0.00 | 1.05 | 15.91 | 29.62 | 31.07 | 304.34 | 0.6033 | -809.0 | -689.0 | |
| 0.00 | 1.96 | 0.00 | 1.21 | 15.86 | 29.32 | 30.77 | 304.52 | 0.5996 | -893.0 | -754.5 | |
| 0.51 | 2.72 | 0.31 | 1.63 | 15.73 | 26.66 | 28.11 | 306.70 | 0.5678 | 848.3 | 650.9 | |
| 0.00 | 1.79 | 0.00 | 1.06 | 15.99 | 25.38 | 26.83 | 308.34 | 0.5554 | -883.0 | -731.1 | |
| 0.00 | 0.77 | 0.00 | 0.46 | 16.99 | 25.16 | 26.60 | 310.02 | 0.5615 | 500.0 | 426.7 | |
| 0.00 | 1.79 | 0.00 | 1.08 | 18.37 | 25.28 | 26.72 | 311.82 | 0.5749 | 188.0 | 261.0 | |
| 0.00 | 2.72 | 0.00 | 1.62 | 17.29 | 24.65 | 26.10 | 310.98 | 0.5586 | 947.0 | 706.2 | |
| 0.00 | 1.87 | 0.00 | 1.11 | 17.10 | 24.52 | 25.97 | 310.84 | 0.5553 | 854.0 | 776.3 | |
| 0.00 | 1.02 | 0.00 | 0.61 | 17.00 | 24.37 | 25.81 | 310.86 | 0.5528 | 782.0 | 575.1 | |
| 0.00 | 0.77 | 0.00 | 0.45 | 16.17 | 24.24 | 25.69 | 309.79 | 0.5441 | 811.0 | 618.1 | |
| 0.00 | 1.45 | 0.00 | 0.85 | 15.88 | 23.83 | 25.28 | 309.80 | 0.5367 | 835.0 | 668.0 | |
| 0.00 | 2.64 | 0.00 | 1.54 | 15.85 | 23.18 | 24.63 | 310.48 | 0.5292 | 889.0 | 792.5 | |
| 0.85 | 1.70 | 0.50 | 0.99 | 16.34 | 22.67 | 24.12 | 311.78 | 0.5280 | 836.0 | 752.1 | |
| 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. | |