| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.73 | 0.00 | 11.09 | 5.57 | 25.47 | 6.40 | 331.45 | 0.2418 | -49.0 | -94.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.25 | 0.00 | 1.66 | 3.60 | 29.13 | 10.06 | 314.27 | 0.2445 | -787.0 | -734.7 | |
| 0.00 | 0.79 | 0.00 | 0.40 | 4.50 | 28.38 | 9.31 | 319.02 | 0.2469 | -698.0 | -535.0 | |
| 0.00 | 1.06 | 0.00 | 0.54 | 6.12 | 28.28 | 9.21 | 323.28 | 0.2673 | -682.0 | -609.8 | |
| 0.00 | 1.32 | 0.00 | 0.67 | 3.58 | 28.03 | 8.96 | 317.55 | 0.2313 | -777.0 | -624.5 | |
| 0.00 | 1.32 | 0.00 | 0.67 | 2.16 | 26.86 | 7.79 | 317.10 | 0.2000 | -757.0 | -571.0 | |
| 0.00 | 2.20 | 0.00 | 1.12 | 4.22 | 26.22 | 7.14 | 325.64 | 0.2208 | -833.0 | -680.4 | |
| 0.00 | 1.32 | 0.00 | 0.67 | 3.98 | 26.21 | 7.14 | 325.02 | 0.2173 | -808.0 | -642.5 | |
| 0.00 | 0.44 | 0.00 | 0.23 | 8.14 | 25.12 | 6.04 | 337.24 | 0.2706 | 534.0 | 590.2 | |
| 0.00 | 1.32 | 0.00 | 0.67 | 4.30 | 25.01 | 5.94 | 330.61 | 0.2110 | -815.0 | -659.9 | |
| 0.00 | 1.23 | 0.00 | 0.63 | 7.61 | 24.92 | 5.85 | 337.12 | 0.2612 | 776.0 | 687.0 | |
| 0.00 | 2.29 | 0.00 | 1.17 | 7.86 | 24.69 | 5.61 | 338.32 | 0.2635 | 851.0 | 683.4 | |
| 0.00 | 1.58 | 0.00 | 0.81 | 8.29 | 24.57 | 5.50 | 339.31 | 0.2696 | 748.0 | 652.2 | |
| 0.00 | 1.49 | 0.00 | 0.77 | 8.87 | 23.57 | 4.50 | 343.45 | 0.2735 | 746.0 | 628.0 | |
| 0.00 | 1.06 | 0.00 | 0.54 | 6.05 | 17.39 | -1.68 | 7.79 | 0.2165 | 856.0 | 632.2 | |
| 0.00 | 1.06 | 0.00 | 0.54 | 7.25 | 17.02 | -2.05 | 8.62 | 0.2377 | 911.0 | 798.2 | |
| 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. | |