| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.16 | 119.11 | 26.60 | 102.92 | 7.04 | 211.03 | 55.44 | 273.96 | 0.8209 | 12.9 | -80.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.07 | 70.87 | 8.20 | 63.77 | 7.35 | 212.83 | 57.25 | 274.47 | 0.8388 | -704.6 | -282.9 | |
| 6.34 | -1.00 | 5.67 | -1.00 | 7.24 | 212.47 | 56.89 | 274.31 | 0.8354 | -923.8 | 999999 | |
| 0.00 | 0.62 | 0.00 | 0.53 | 7.13 | 211.14 | 55.55 | 274.09 | 0.8225 | -649.0 | -527.1 | |
| 0.00 | 1.23 | 0.00 | 1.07 | 7.28 | 211.11 | 55.52 | 274.27 | 0.8222 | -632.0 | -534.6 | |
| 0.00 | 1.14 | 0.00 | 0.98 | 6.27 | 210.62 | 55.03 | 273.00 | 0.8178 | -502.0 | -345.5 | |
| 0.00 | 0.97 | 0.00 | 0.80 | 7.20 | 209.10 | 53.51 | 274.04 | 0.8019 | 310.0 | 245.5 | |
| 0.00 | 1.06 | 0.00 | 0.87 | 6.70 | 208.92 | 53.33 | 273.41 | 0.8003 | 146.0 | 108.8 | |
| 0.00 | 1.14 | 0.00 | 0.94 | 6.89 | 208.80 | 53.21 | 273.64 | 0.7989 | 354.0 | 300.2 | |
| 0.00 | 1.76 | 0.00 | 1.44 | 7.08 | 208.73 | 53.14 | 273.87 | 0.7980 | 615.0 | 474.2 | |
| 9.68 | 19.37 | 7.88 | 15.77 | 6.41 | 208.47 | 52.88 | 273.01 | 0.7957 | 590.9 | 151.1 | |
| 0.35 | 1.32 | 0.28 | 1.06 | 6.39 | 208.01 | 52.43 | 272.96 | 0.7909 | 554.2 | 507.8 | |
| 0.00 | 1.94 | 0.00 | 1.56 | 6.75 | 208.07 | 52.48 | 273.41 | 0.7913 | 523.0 | 475.6 | |
| 0.00 | 1.06 | 0.00 | 0.85 | 6.93 | 208.10 | 52.51 | 273.64 | 0.7915 | 379.0 | 303.8 | |
| 0.00 | 1.06 | 0.00 | 0.85 | 6.14 | 207.78 | 52.19 | 272.62 | 0.7886 | 503.0 | 479.3 | |
| 0.00 | 1.14 | 0.00 | 0.92 | 6.36 | 207.71 | 52.12 | 272.89 | 0.7877 | 676.0 | 580.7 | |
| 4.49 | 12.41 | 3.59 | 9.92 | 6.66 | 207.66 | 52.07 | 273.28 | 0.7870 | 839.4 | 652.2 | |
| 1.23 | -16.00 | 0.98 | -16.00 | 6.49 | 207.53 | 51.95 | 273.05 | 0.7857 | 793.4 | 999999 | |
| 0.00 | 2.02 | 0.00 | 1.59 | 7.13 | 206.85 | 51.26 | 273.82 | 0.7780 | 647.0 | 546.9 | |
| 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. | |