| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 51.04 | 343.38 | 31.99 | 214.85 | 17.88 | 166.37 | 30.47 | 307.85 | 0.6133 | -773.1 | -347.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 51.04 | 326.32 | 31.99 | 204.45 | 17.86 | 166.52 | 30.62 | 307.69 | 0.6148 | -1280.4 | -394.8 | |
| 0.00 | 0.89 | 0.00 | 0.55 | 17.35 | 165.22 | 29.31 | 308.15 | 0.5965 | -371.0 | -257.9 | |
| 0.00 | 1.51 | 0.00 | 0.93 | 17.51 | 164.53 | 28.62 | 309.03 | 0.5902 | -278.0 | -100.7 | |
| 0.00 | 1.60 | 0.00 | 0.98 | 17.28 | 164.45 | 28.54 | 308.78 | 0.5875 | 528.0 | 378.6 | |
| 0.00 | 1.24 | 0.00 | 0.77 | 18.23 | 164.44 | 28.53 | 310.09 | 0.5952 | 609.0 | 426.6 | |
| 0.00 | 1.33 | 0.00 | 0.81 | 17.50 | 163.48 | 27.58 | 310.02 | 0.5787 | 619.0 | 512.7 | |
| 0.00 | 0.71 | 0.00 | 0.43 | 17.86 | 163.33 | 27.42 | 310.66 | 0.5801 | 611.0 | 563.4 | |
| 0.00 | 0.53 | 0.00 | 0.32 | 18.31 | 163.26 | 27.36 | 311.35 | 0.5834 | 141.0 | 178.2 | |
| 0.00 | 2.31 | 0.00 | 1.40 | 17.82 | 163.11 | 27.20 | 310.83 | 0.5773 | 873.0 | 675.1 | |
| 0.00 | 1.33 | 0.00 | 0.81 | 18.43 | 162.93 | 27.02 | 311.85 | 0.5808 | 582.0 | 473.7 | |
| 0.00 | 1.69 | 0.00 | 1.02 | 18.19 | 162.71 | 26.80 | 311.75 | 0.5764 | 832.0 | 743.9 | |
| 0.00 | 1.96 | 0.00 | 1.19 | 18.65 | 162.68 | 26.77 | 312.40 | 0.5802 | 718.0 | 563.9 | |
| 0.00 | 0.98 | 0.00 | 0.60 | 21.11 | 162.12 | 26.22 | 316.17 | 0.5973 | 587.0 | 484.1 | |
| 0.00 | 0.98 | 0.00 | 0.59 | 19.40 | 161.56 | 25.65 | 314.58 | 0.5755 | 725.0 | 618.5 | |
| 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. | |