| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.93 | 431.12 | 36.70 | 226.43 | 12.51 | 13.63 | -4.33 | 12.95 | 0.3317 | -876.1 | -385.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.58 | 407.28 | 36.52 | 213.93 | 12.59 | 13.76 | -4.20 | 12.49 | 0.3323 | -1358.8 | -435.1 | |
| 0.00 | 1.50 | 0.00 | 0.76 | 3.79 | 12.94 | -5.03 | 26.63 | 0.1959 | 844.0 | 639.5 | |
| 0.00 | 2.02 | 0.00 | 1.05 | 9.52 | 12.58 | -5.38 | 18.81 | 0.2883 | 886.0 | 621.1 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 11.40 | 12.43 | -5.54 | 17.33 | 0.3190 | -670.0 | -520.5 | |
| 0.35 | 1.41 | 0.18 | 0.74 | 11.82 | 11.99 | -5.98 | 18.20 | 0.3277 | -601.2 | -511.5 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 10.12 | 12.02 | -5.94 | 19.90 | 0.3009 | 748.0 | 652.7 | |
| 0.00 | 1.58 | 0.00 | 0.85 | 15.42 | 11.78 | -6.19 | 15.73 | 0.3852 | 688.0 | 559.1 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 12.29 | 11.83 | -6.14 | 18.21 | 0.3360 | -633.0 | -483.1 | |
| 0.00 | 2.99 | 0.00 | 1.57 | 12.01 | 11.49 | -6.47 | 19.40 | 0.3334 | -668.0 | -530.6 | |
| 0.00 | 2.20 | 0.00 | 1.15 | 11.42 | 11.32 | -6.65 | 20.52 | 0.3251 | 717.0 | 590.9 | |
| 0.00 | 1.76 | 0.00 | 0.92 | 11.55 | 11.01 | -6.96 | 21.24 | 0.3290 | 867.0 | 714.1 | |
| 0.00 | 1.85 | 0.00 | 0.97 | 11.77 | 10.91 | -7.06 | 21.27 | 0.3330 | 723.0 | 542.2 | |
| 0.00 | 3.34 | 0.00 | 1.76 | 11.93 | 10.63 | -7.34 | 21.85 | 0.3372 | 916.0 | 745.8 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 10.69 | 9.37 | -8.60 | 26.82 | 0.3271 | 723.0 | 618.2 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 11.14 | 8.95 | -9.02 | 27.29 | 0.3368 | 770.0 | 635.4 | |
| 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. | |