| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 28.51 | 0.00 | 14.69 | 17.55 | 322.95 | 10.24 | 321.81 | 0.2772 | 733.5 | 637.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.30 | 0.00 | 0.68 | 17.00 | 325.11 | 12.40 | 315.14 | 0.2925 | -746.0 | -559.7 | |
| 0.00 | 6.52 | 0.00 | 3.38 | 17.59 | 324.90 | 12.19 | 317.06 | 0.2968 | 773.0 | 689.0 | |
| 0.00 | 2.00 | 0.00 | 1.04 | 17.74 | 324.62 | 11.91 | 318.08 | 0.2955 | 864.0 | 726.1 | |
| 0.00 | 1.56 | 0.00 | 0.81 | 17.90 | 324.44 | 11.73 | 318.87 | 0.2954 | 805.0 | 671.2 | |
| 0.00 | 2.78 | 0.00 | 1.44 | 18.09 | 324.26 | 11.55 | 319.72 | 0.2958 | 1082.0 | 883.6 | |
| 0.00 | 1.56 | 0.00 | 0.81 | 18.43 | 324.12 | 11.41 | 320.82 | 0.2985 | 957.0 | 789.0 | |
| 0.00 | 1.13 | 0.00 | 0.58 | 15.29 | 323.80 | 11.10 | 313.59 | 0.2575 | 809.0 | 572.1 | |
| 0.00 | 1.39 | 0.00 | 0.70 | 12.50 | 321.34 | 8.64 | 311.09 | 0.1954 | 866.0 | 734.7 | |
| 0.00 | 3.13 | 0.00 | 1.60 | 17.19 | 321.00 | 8.29 | 326.54 | 0.2510 | 813.0 | 618.2 | |
| 0.00 | 1.83 | 0.00 | 0.93 | 16.61 | 320.66 | 7.95 | 326.28 | 0.2399 | 878.0 | 722.9 | |
| 0.00 | 1.48 | 0.00 | 0.75 | 16.46 | 320.53 | 7.82 | 326.34 | 0.2365 | 569.0 | 525.0 | |
| 0.00 | 1.65 | 0.00 | 0.85 | 19.92 | 320.53 | 7.82 | 333.35 | 0.2864 | 939.0 | 718.6 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 20.27 | 320.06 | 7.36 | 335.25 | 0.2882 | 876.0 | 652.5 | |
| 0.00 | 1.22 | 0.00 | 0.63 | 20.87 | 318.78 | 6.07 | 339.94 | 0.2892 | 784.0 | 580.5 | |
| 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. | |