| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.76 | 0.00 | 9.75 | 18.15 | 342.16 | -21.25 | 52.86 | 0.4329 | -269.9 | -339.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.07 | 0.00 | 1.12 | 18.70 | 344.10 | -19.31 | 49.43 | 0.4140 | -745.0 | -641.5 | |
| 0.00 | 1.64 | 0.00 | 0.89 | 18.95 | 344.07 | -19.33 | 49.00 | 0.4167 | -895.0 | -760.9 | |
| 0.00 | 1.90 | 0.00 | 1.02 | 16.41 | 344.28 | -19.12 | 53.89 | 0.3906 | -914.0 | -762.0 | |
| 0.00 | 0.86 | 0.00 | 0.46 | 16.31 | 344.13 | -19.27 | 54.30 | 0.3918 | -909.0 | -813.3 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 16.43 | 343.85 | -19.55 | 54.40 | 0.3964 | -832.0 | -664.2 | |
| 0.00 | 1.46 | 0.00 | 0.79 | 16.61 | 343.70 | -19.70 | 54.21 | 0.3999 | -825.0 | -635.2 | |
| 0.00 | 1.46 | 0.00 | 0.79 | 16.36 | 343.63 | -19.77 | 54.83 | 0.3988 | -765.0 | -703.6 | |
| 0.00 | 2.07 | 0.00 | 1.12 | 16.93 | 342.87 | -20.53 | 54.58 | 0.4134 | -838.0 | -598.9 | |
| 0.00 | 0.78 | 0.00 | 0.42 | 16.99 | 342.70 | -20.70 | 54.67 | 0.4161 | -689.0 | -473.9 | |
| 0.00 | 0.86 | 0.00 | 0.49 | 22.52 | 341.49 | -21.91 | 46.04 | 0.4809 | 704.0 | 619.5 | |
| 0.00 | 1.21 | 0.00 | 0.68 | 22.00 | 340.81 | -22.59 | 47.69 | 0.4835 | 800.0 | 625.0 | |
| 0.00 | 0.86 | 0.00 | 0.49 | 19.42 | 337.07 | -26.34 | 55.95 | 0.5070 | 853.0 | 696.4 | |
| 0.00 | 0.78 | 0.00 | 0.45 | 20.22 | 336.53 | -26.87 | 55.06 | 0.5194 | 629.0 | 474.1 | |
| 0.00 | 0.78 | 0.00 | 0.47 | 19.03 | 331.41 | -31.99 | 60.90 | 0.5755 | 648.0 | 550.0 | |
| 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. | |