| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.43 | 0.00 | 14.33 | -5.20 | 139.06 | -25.89 | 113.98 | 0.4781 | -730.3 | -623.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.41 | 0.00 | 0.78 | -4.16 | 140.82 | -24.13 | 113.51 | 0.4465 | -745.0 | -606.1 | |
| 0.00 | 2.11 | 0.00 | 1.17 | -4.33 | 140.45 | -24.50 | 113.52 | 0.4529 | -786.0 | -634.2 | |
| 0.00 | 1.76 | 0.00 | 0.98 | -4.61 | 139.81 | -25.14 | 113.50 | 0.4637 | -848.0 | -693.1 | |
| 0.00 | 1.67 | 0.00 | 0.93 | -4.00 | 139.67 | -25.29 | 112.18 | 0.4620 | -722.0 | -577.3 | |
| 0.00 | 1.14 | 0.00 | 0.65 | -5.77 | 139.22 | -25.73 | 115.23 | 0.4794 | -837.0 | -728.1 | |
| 0.00 | 3.79 | 0.00 | 2.13 | -5.47 | 139.14 | -25.81 | 114.58 | 0.4786 | -831.0 | -683.1 | |
| 0.00 | 1.58 | 0.00 | 0.89 | -4.64 | 139.17 | -25.78 | 113.02 | 0.4729 | -533.0 | -497.8 | |
| 0.00 | 3.52 | 0.00 | 1.99 | -6.43 | 138.99 | -25.97 | 116.25 | 0.4871 | -843.0 | -620.4 | |
| 0.00 | 1.14 | 0.00 | 0.65 | -6.12 | 138.97 | -25.98 | 115.66 | 0.4852 | -641.0 | -619.2 | |
| 0.00 | 2.20 | 0.00 | 1.23 | -3.27 | 139.06 | -25.90 | 110.22 | 0.4666 | -851.0 | -726.0 | |
| 0.00 | 1.94 | 0.00 | 1.10 | -6.51 | 138.51 | -26.44 | 115.98 | 0.4941 | -634.0 | -537.5 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -7.30 | 138.09 | -26.86 | 117.03 | 0.5052 | -622.0 | -510.2 | |
| 0.00 | 0.97 | 0.00 | 0.55 | -3.51 | 136.85 | -28.10 | 109.08 | 0.4995 | -643.0 | -577.7 | |
| 0.00 | 1.23 | 0.00 | 0.72 | -6.15 | 136.11 | -28.84 | 113.36 | 0.5245 | -688.0 | -560.9 | |
| 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. | |