| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.72 | 28.07 | 2.96 | 14.52 | 16.61 | 22.50 | 9.66 | 325.66 | 0.2924 | -154.6 | -190.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.09 | 0.00 | 0.57 | 13.37 | 26.80 | 13.96 | 307.87 | 0.2986 | 801.0 | 569.1 | |
| 1.73 | 1.91 | 0.90 | 0.99 | 13.52 | 26.61 | 13.78 | 308.65 | 0.2978 | 999.7 | 930.0 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 15.19 | 25.32 | 12.49 | 315.64 | 0.2997 | -845.0 | -588.8 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 15.56 | 25.15 | 12.31 | 316.92 | 0.3022 | -950.0 | -833.2 | |
| 0.00 | 2.00 | 0.00 | 1.04 | 16.54 | 24.99 | 12.15 | 319.50 | 0.3120 | -885.0 | -618.5 | |
| 0.00 | 0.54 | 0.00 | 0.28 | 14.45 | 23.77 | 10.93 | 317.52 | 0.2732 | -812.0 | -598.7 | |
| 0.00 | 2.09 | 0.00 | 1.08 | 16.71 | 23.67 | 10.83 | 323.01 | 0.3004 | -1026.0 | -825.1 | |
| 0.00 | 3.09 | 0.00 | 1.59 | 15.80 | 22.78 | 9.94 | 323.38 | 0.2797 | -931.0 | -803.6 | |
| 0.00 | 0.64 | 0.00 | 0.33 | 16.09 | 22.60 | 9.76 | 324.48 | 0.2817 | -699.0 | -519.3 | |
| 0.00 | 1.73 | 0.00 | 0.89 | 16.37 | 22.00 | 9.16 | 326.75 | 0.2799 | -911.0 | -642.5 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 17.39 | 21.02 | 8.18 | 331.50 | 0.2858 | 958.0 | 799.1 | |
| 2.36 | 3.00 | 1.22 | 1.55 | 16.98 | 20.90 | 8.07 | 331.10 | 0.2789 | 952.1 | 814.1 | |
| 1.63 | 3.81 | 0.84 | 1.96 | 16.76 | 20.48 | 7.64 | 332.00 | 0.2723 | 874.1 | 877.7 | |
| 0.00 | 1.91 | 0.00 | 0.98 | 17.45 | 20.47 | 7.64 | 333.22 | 0.2825 | 968.0 | 787.0 | |
| 0.00 | 1.82 | 0.00 | 0.96 | 23.52 | 17.21 | 4.37 | 348.77 | 0.3601 | -777.0 | -576.3 | |
| 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. | |