| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.51 | 0.00 | 9.54 | -20.81 | 79.86 | -18.05 | 145.89 | 0.5113 | 603.6 | 514.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.48 | -19.95 | 84.47 | -13.43 | 151.72 | 0.4629 | 731.0 | 525.3 | |
| 0.00 | 2.33 | 0.00 | 1.28 | -17.53 | 84.51 | -13.40 | 148.96 | 0.4302 | 906.0 | 653.4 | |
| 0.00 | 1.30 | 0.00 | 0.74 | -22.14 | 83.24 | -14.67 | 151.95 | 0.5009 | 488.0 | 442.7 | |
| 0.00 | 1.64 | 0.00 | 0.93 | -20.82 | 83.05 | -14.86 | 150.26 | 0.4851 | 680.0 | 525.1 | |
| 0.00 | 1.30 | 0.00 | 0.73 | -20.86 | 82.88 | -15.03 | 150.02 | 0.4869 | 778.0 | 672.1 | |
| 0.00 | 1.04 | 0.00 | 0.59 | -20.50 | 82.85 | -15.06 | 149.57 | 0.4825 | 587.0 | 499.8 | |
| 0.00 | 1.12 | 0.00 | 0.64 | -20.54 | 82.55 | -15.36 | 149.13 | 0.4853 | 812.0 | 519.8 | |
| 0.00 | 0.78 | 0.00 | 0.45 | -20.39 | 78.84 | -19.06 | 143.33 | 0.5147 | 731.0 | 642.3 | |
| 0.00 | 0.86 | 0.00 | 0.52 | -22.82 | 76.54 | -21.37 | 143.18 | 0.5625 | 400.0 | 389.0 | |
| 0.00 | 1.04 | 0.00 | 0.61 | -20.24 | 76.77 | -21.14 | 140.33 | 0.5322 | 305.0 | 464.9 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -20.71 | 76.60 | -21.31 | 140.70 | 0.5388 | 511.0 | 399.0 | |
| 0.00 | 0.78 | 0.00 | 0.46 | -20.55 | 76.14 | -21.76 | 139.93 | 0.5414 | 676.0 | 613.4 | |
| 0.00 | 1.30 | 0.00 | 0.76 | -20.63 | 75.82 | -22.08 | 139.62 | 0.5452 | 350.0 | 345.4 | |
| 0.00 | 1.21 | 0.00 | 0.79 | -25.49 | 68.94 | -28.97 | 138.02 | 0.6560 | 495.0 | 437.6 | |
| 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. | |