| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 26.71 | 0.00 | 13.38 | 9.96 | 183.08 | -1.96 | 260.84 | 0.0938 | -432.1 | -482.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.32 | 0.00 | 1.15 | 10.83 | 187.49 | 2.46 | 326.27 | 0.0762 | -718.0 | -590.8 | |
| 0.00 | 2.86 | 0.00 | 1.42 | 6.08 | 187.21 | 2.18 | 242.43 | 0.0428 | -1009.0 | -937.8 | |
| 0.00 | 1.16 | 0.00 | 0.58 | 11.71 | 187.10 | 2.06 | 335.77 | 0.0863 | -770.0 | -485.8 | |
| 0.00 | 1.25 | 0.00 | 0.62 | 8.17 | 186.74 | 1.70 | 299.56 | 0.0339 | -903.0 | -639.8 | |
| 0.00 | 1.16 | 0.00 | 0.58 | 5.70 | 185.87 | 0.84 | 208.76 | 0.0304 | -1073.0 | -885.8 | |
| 0.00 | 1.97 | 0.00 | 0.98 | 10.87 | 185.83 | 0.80 | 347.91 | 0.0654 | -987.0 | -801.8 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 12.08 | 185.74 | 0.71 | 351.89 | 0.0860 | -818.0 | -591.5 | |
| 0.00 | 2.32 | 0.00 | 1.15 | 11.02 | 185.28 | 0.24 | 356.43 | 0.0667 | -1099.0 | -842.2 | |
| 0.00 | 1.16 | 0.00 | 0.58 | 11.56 | 185.15 | 0.12 | 358.46 | 0.0762 | -956.0 | -834.8 | |
| 0.00 | 2.59 | 0.00 | 1.28 | 5.97 | 184.96 | -0.07 | 176.73 | 0.0219 | -738.0 | -625.0 | |
| 0.00 | 1.34 | 0.00 | 0.67 | 11.32 | 184.84 | -0.19 | 2.59 | 0.0720 | -859.0 | -777.3 | |
| 0.00 | 1.34 | 0.00 | 0.67 | 10.72 | 184.81 | -0.22 | 3.54 | 0.0614 | -852.0 | -775.2 | |
| 0.00 | 1.34 | 0.00 | 0.67 | 10.05 | 183.74 | -1.29 | 24.23 | 0.0545 | -757.0 | -518.3 | |
| 0.00 | 1.43 | 0.00 | 0.71 | 9.25 | 180.89 | -4.14 | 63.36 | 0.0802 | 869.0 | 535.1 | |
| 0.00 | 1.07 | 0.00 | 0.53 | 10.11 | 178.82 | -6.22 | 64.39 | 0.1188 | 878.0 | 737.9 | |
| 0.00 | 1.43 | 0.00 | 0.76 | 12.82 | 163.98 | -21.06 | 73.20 | 0.3675 | 664.0 | 539.6 | |
| 0.00 | 0.45 | 0.00 | 0.24 | 15.78 | 162.60 | -22.43 | 66.71 | 0.4014 | 690.0 | 617.2 | |
| 0.00 | 0.54 | 0.00 | 0.30 | 21.64 | 160.13 | -24.90 | 56.41 | 0.4718 | 661.0 | 414.0 | |
| 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. | |