| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.31 | 43.01 | 5.78 | 22.05 | 18.22 | 324.23 | -7.14 | 27.26 | 0.2547 | 648.2 | 301.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.57 | 10.01 | 1.81 | 5.08 | 16.95 | 326.72 | -4.66 | 21.08 | 0.2169 | -1115.1 | -829.9 | |
| 1.04 | 3.40 | 0.53 | 1.72 | 17.16 | 326.40 | -4.97 | 22.00 | 0.2222 | -1016.4 | -846.0 | |
| 0.00 | 2.70 | 0.00 | 1.38 | 18.18 | 325.20 | -6.17 | 24.63 | 0.2462 | 915.0 | 676.6 | |
| 0.00 | 1.13 | 0.00 | 0.57 | 13.96 | 324.99 | -6.38 | 35.64 | 0.1859 | 869.0 | 703.3 | |
| 0.00 | 0.70 | 0.00 | 0.36 | 17.60 | 324.78 | -6.59 | 27.20 | 0.2404 | 1033.0 | 777.9 | |
| 1.48 | 6.18 | 0.76 | 3.17 | 18.82 | 324.00 | -7.37 | 27.45 | 0.2645 | 1093.7 | 830.8 | |
| 3.48 | 6.53 | 1.79 | 3.35 | 18.54 | 323.92 | -7.45 | 28.23 | 0.2611 | 1095.8 | 1134.3 | |
| 1.74 | -7.00 | 0.89 | -7.00 | 18.32 | 323.87 | -7.50 | 28.82 | 0.2584 | 1137.8 | 999999 | |
| 0.00 | 1.04 | 0.00 | 0.54 | 18.50 | 323.54 | -7.83 | 29.48 | 0.2637 | 874.0 | 753.7 | |
| 0.00 | 2.44 | 0.00 | 1.25 | 18.17 | 323.56 | -7.81 | 30.11 | 0.2587 | 857.0 | 631.2 | |
| 0.00 | 1.13 | 0.00 | 0.58 | 19.11 | 322.75 | -8.62 | 30.67 | 0.2790 | 745.0 | 707.3 | |
| 0.00 | 1.74 | 0.00 | 0.90 | 18.58 | 322.61 | -8.76 | 32.10 | 0.2728 | 918.0 | 724.8 | |
| 0.00 | 0.61 | 0.00 | 0.31 | 18.89 | 322.34 | -9.03 | 32.25 | 0.2795 | 768.0 | 638.3 | |
| 0.00 | 1.92 | 0.00 | 1.01 | 21.77 | 320.70 | -10.67 | 31.17 | 0.3337 | 816.0 | 633.3 | |
| 0.00 | 0.87 | 0.00 | 0.46 | 20.20 | 319.81 | -11.56 | 36.07 | 0.3208 | 799.0 | 682.8 | |
| 0.00 | 1.57 | 0.00 | 0.82 | 20.44 | 319.40 | -11.97 | 36.52 | 0.3279 | 760.0 | 597.9 | |
| 0.00 | 1.04 | 0.00 | 0.55 | 19.51 | 319.09 | -12.28 | 39.10 | 0.3194 | 922.0 | 638.8 | |
| 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. | |