| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66.43 | 383.11 | 35.27 | 203.45 | -1.41 | 154.77 | 19.51 | 248.40 | 0.3606 | 1021.1 | 400.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.69 | 320.18 | 28.56 | 170.39 | -1.41 | 155.13 | 19.87 | 248.82 | 0.3660 | 1455.0 | 396.5 | |
| 0.88 | -1.00 | 0.47 | -1.00 | -1.62 | 154.30 | 19.04 | 247.40 | 0.3548 | 974.2 | 999999 | |
| 3.25 | 25.31 | 1.72 | 13.37 | -1.91 | 153.96 | 18.70 | 246.24 | 0.3516 | 994.6 | 687.0 | |
| 2.46 | -3.00 | 1.30 | -3.00 | -1.72 | 153.83 | 18.57 | 246.58 | 0.3484 | 1190.7 | 999999 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -0.45 | 153.69 | 18.44 | 249.87 | 0.3383 | 899.0 | 749.6 | |
| 0.00 | 6.15 | 0.00 | 3.24 | -1.05 | 153.63 | 18.37 | 248.15 | 0.3410 | 728.0 | 870.5 | |
| 0.00 | 3.08 | 0.00 | 1.63 | -4.12 | 153.58 | 18.32 | 240.25 | 0.3627 | 569.0 | 459.4 | |
| 0.00 | 1.41 | 0.00 | 0.74 | -0.14 | 153.54 | 18.28 | 250.56 | 0.3340 | 706.0 | 525.6 | |
| 0.00 | 1.76 | 0.00 | 0.92 | 0.19 | 153.41 | 18.15 | 251.39 | 0.3302 | 474.0 | 335.4 | |
| 6.15 | 12.48 | 3.22 | 6.54 | -0.25 | 153.13 | 17.87 | 249.82 | 0.3283 | 1103.8 | 757.2 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -3.31 | 153.09 | 17.83 | 241.56 | 0.3492 | 695.0 | 562.1 | |
| 0.00 | 1.32 | 0.00 | 0.69 | -0.02 | 151.74 | 16.49 | 248.89 | 0.3056 | 752.0 | 649.1 | |
| 0.00 | 1.05 | 0.00 | 0.55 | 0.20 | 151.43 | 16.17 | 249.18 | 0.2993 | -46.0 | -208.2 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -1.91 | 150.41 | 15.15 | 241.30 | 0.2992 | -685.0 | -597.6 | |
| 0.00 | 1.23 | 0.00 | 0.64 | -1.72 | 150.07 | 14.81 | 241.30 | 0.2926 | -731.0 | -575.3 | |
| 0.00 | 2.11 | 0.00 | 1.09 | -2.35 | 150.01 | 14.75 | 239.34 | 0.2971 | -1013.0 | -859.9 | |
| 0.00 | 1.49 | 0.00 | 0.77 | -1.50 | 149.85 | 14.59 | 241.59 | 0.2876 | -913.0 | -810.6 | |
| 0.00 | 2.90 | 0.00 | 1.50 | -1.80 | 149.73 | 14.47 | 240.48 | 0.2883 | -926.0 | -827.3 | |
| 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. | |