| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.95 | 80.71 | 15.02 | 41.94 | 6.42 | 11.33 | 11.07 | 321.16 | 0.3045 | 167.5 | -63.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.69 | 3.38 | 0.36 | 1.77 | 5.58 | 14.84 | 14.57 | 311.02 | 0.3334 | -861.0 | -635.1 | |
| 0.00 | 1.21 | 0.00 | 0.64 | 5.81 | 14.47 | 14.21 | 312.28 | 0.3315 | -836.0 | -634.3 | |
| 1.39 | 9.10 | 0.73 | 4.77 | 6.20 | 14.02 | 13.76 | 314.06 | 0.3305 | -895.0 | -536.0 | |
| 0.52 | -3.00 | 0.27 | -3.00 | 6.32 | 13.90 | 13.64 | 314.57 | 0.3304 | -866.7 | 999999 | |
| 7.02 | 16.47 | 3.68 | 8.62 | 6.36 | 13.35 | 13.08 | 315.87 | 0.3246 | -976.1 | -851.1 | |
| 1.39 | 5.98 | 0.72 | 3.12 | 6.70 | 12.31 | 12.05 | 318.96 | 0.3172 | -952.2 | -651.5 | |
| 0.00 | 1.65 | 0.00 | 0.86 | 7.01 | 12.23 | 11.97 | 319.79 | 0.3201 | -740.0 | -487.3 | |
| 0.00 | 1.13 | 0.00 | 0.58 | 5.55 | 11.77 | 11.50 | 317.81 | 0.2968 | 740.0 | 626.2 | |
| 0.00 | 0.95 | 0.00 | 0.49 | 5.28 | 10.48 | 10.22 | 320.57 | 0.2794 | 582.0 | 465.6 | |
| 0.00 | 1.91 | 0.00 | 0.99 | 6.66 | 10.45 | 10.18 | 323.60 | 0.2973 | 801.0 | 725.0 | |
| 0.69 | 2.25 | 0.36 | 1.17 | 7.17 | 10.09 | 9.83 | 325.56 | 0.3009 | -734.5 | -613.3 | |
| 0.00 | 2.17 | 0.00 | 1.12 | 6.68 | 10.08 | 9.82 | 324.64 | 0.2940 | 822.0 | 650.5 | |
| 0.00 | 2.08 | 0.00 | 1.07 | 5.81 | 9.73 | 9.47 | 323.87 | 0.2788 | 952.0 | 721.6 | |
| 2.34 | 28.87 | 1.21 | 14.91 | 6.73 | 9.48 | 9.21 | 326.45 | 0.2890 | 846.4 | 713.4 | |
| 10.66 | -14.00 | 5.50 | -14.00 | 6.42 | 9.20 | 8.93 | 326.66 | 0.2821 | 1085.7 | 999999 | |
| 4.25 | -14.00 | 2.19 | -14.00 | 6.72 | 9.14 | 8.88 | 327.41 | 0.2859 | 858.4 | 999999 | |
| 0.00 | 2.43 | 0.00 | 1.25 | 6.62 | 8.72 | 8.45 | 328.50 | 0.2807 | 763.0 | 649.2 | |
| 0.00 | 1.13 | 0.00 | 0.58 | 6.32 | 8.71 | 8.45 | 327.93 | 0.2762 | 768.0 | 679.3 | |
| 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. | |