| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.68 | 63.83 | 20.43 | 44.22 | -17.96 | 157.99 | -36.94 | 125.11 | 0.7007 | 229.5 | -115.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.98 | 0.00 | 0.67 | -18.18 | 159.71 | -35.22 | 126.62 | 0.6849 | 434.0 | 362.1 | |
| 10.01 | 27.54 | 6.76 | 18.61 | -17.72 | 159.66 | -35.27 | 126.01 | 0.6822 | 887.5 | 430.3 | |
| 7.33 | -2.00 | 4.95 | -2.00 | -17.40 | 159.50 | -35.43 | 125.50 | 0.6817 | 881.4 | 999999 | |
| 0.80 | -2.00 | 0.54 | -2.00 | -17.19 | 159.23 | -35.69 | 125.04 | 0.6830 | 636.7 | 999999 | |
| 0.00 | 2.59 | 0.00 | 1.74 | -16.39 | 159.41 | -35.52 | 124.15 | 0.6758 | 644.0 | 513.0 | |
| 0.45 | 1.70 | 0.30 | 1.15 | -17.02 | 158.84 | -36.09 | 124.54 | 0.6860 | 500.0 | 398.9 | |
| 0.00 | 1.34 | 0.00 | 0.93 | -17.49 | 157.54 | -37.38 | 124.19 | 0.7024 | 579.0 | 315.3 | |
| 0.54 | 5.27 | 0.38 | 3.76 | -18.96 | 156.60 | -38.33 | 125.32 | 0.7212 | -709.5 | -563.2 | |
| 2.41 | 21.90 | 1.71 | 15.58 | -18.36 | 156.64 | -38.29 | 124.63 | 0.7170 | -906.8 | -650.3 | |
| 5.90 | -9.00 | 4.20 | -9.00 | -18.58 | 156.33 | -38.60 | 124.69 | 0.7215 | -752.6 | 999999 | |
| 0.72 | -9.00 | 0.51 | -9.00 | -18.17 | 156.44 | -38.49 | 124.27 | 0.7178 | -812.6 | 999999 | |
| 0.00 | 1.88 | 0.00 | 1.34 | -18.86 | 156.21 | -38.71 | 124.94 | 0.7243 | -308.0 | -218.7 | |
| 1.52 | -9.00 | 1.08 | -9.00 | -18.09 | 156.26 | -38.67 | 124.05 | 0.7191 | -758.2 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.44 | -16.00 | 155.23 | -39.69 | 120.83 | 0.7173 | 513.0 | 461.1 | |
| 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. | |