| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.92 | 0.00 | 14.05 | 14.40 | 57.79 | 27.53 | 289.50 | 0.4760 | 54.6 | 66.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.40 | 0.00 | 0.86 | 11.53 | 66.48 | 36.22 | 281.28 | 0.5925 | -641.0 | -557.2 | |
| 0.00 | 0.70 | 0.00 | 0.43 | 13.56 | 66.47 | 36.21 | 284.68 | 0.5959 | -532.0 | -469.4 | |
| 0.00 | 1.66 | 0.00 | 0.99 | 15.41 | 63.45 | 33.19 | 288.76 | 0.5595 | -497.0 | -453.4 | |
| 0.00 | 0.61 | 0.00 | 0.36 | 15.67 | 63.31 | 33.05 | 289.25 | 0.5584 | -655.0 | -533.4 | |
| 0.00 | 0.79 | 0.00 | 0.45 | 15.68 | 59.18 | 28.91 | 291.12 | 0.5011 | -674.0 | -542.8 | |
| 0.00 | 3.15 | 0.00 | 1.80 | 16.32 | 59.07 | 28.80 | 292.42 | 0.5022 | -661.0 | -584.4 | |
| 0.00 | 1.22 | 0.00 | 0.69 | 13.08 | 58.25 | 27.99 | 286.38 | 0.4784 | 771.0 | 667.4 | |
| 0.00 | 3.06 | 0.00 | 1.72 | 17.13 | 56.87 | 26.60 | 295.36 | 0.4755 | -751.0 | -593.1 | |
| 0.00 | 2.10 | 0.00 | 1.16 | 13.17 | 55.75 | 25.48 | 287.73 | 0.4417 | 738.0 | 584.8 | |
| 0.00 | 0.87 | 0.00 | 0.48 | 13.47 | 55.78 | 25.52 | 288.37 | 0.4433 | 517.0 | 448.5 | |
| 0.00 | 2.80 | 0.00 | 1.54 | 13.24 | 55.45 | 25.19 | 288.05 | 0.4375 | 806.0 | 608.8 | |
| 0.00 | 2.45 | 0.00 | 1.34 | 13.60 | 54.88 | 24.61 | 289.17 | 0.4304 | 752.0 | 671.5 | |
| 0.00 | 1.66 | 0.00 | 0.90 | 13.47 | 53.75 | 23.49 | 289.54 | 0.4130 | 833.0 | 654.9 | |
| 0.00 | 2.45 | 0.00 | 1.33 | 13.73 | 53.31 | 23.05 | 290.45 | 0.4076 | 759.0 | 598.5 | |
| 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. | |