| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.55 | 426.32 | 37.46 | 220.16 | 16.62 | 110.26 | 4.96 | 342.94 | 0.2841 | -1003.7 | -385.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 70.41 | 413.06 | 36.36 | 213.33 | 16.59 | 110.45 | 5.15 | 342.28 | 0.2841 | -1551.9 | -426.2 | |
| 0.26 | -1.00 | 0.13 | -1.00 | 16.22 | 110.07 | 4.77 | 343.12 | 0.2763 | -1339.0 | 999999 | |
| 1.88 | -1.00 | 0.97 | -1.00 | 17.02 | 109.93 | 4.64 | 344.38 | 0.2886 | -923.2 | 999999 | |
| 0.00 | 1.28 | 0.00 | 0.66 | 17.95 | 107.38 | 2.08 | 353.26 | 0.2955 | 893.0 | 783.1 | |
| 0.00 | 1.37 | 0.00 | 0.70 | 16.72 | 107.21 | 1.91 | 353.29 | 0.2747 | 951.0 | 787.4 | |
| 0.00 | 0.85 | 0.00 | 0.44 | 16.84 | 106.81 | 1.51 | 354.73 | 0.2760 | 926.0 | 745.1 | |
| 0.00 | 0.94 | 0.00 | 0.48 | 16.50 | 106.34 | 1.04 | 356.27 | 0.2697 | 797.0 | 596.6 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 17.52 | 105.05 | -0.25 | 0.84 | 0.2863 | 767.0 | 616.8 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 16.97 | 104.98 | -0.31 | 1.08 | 0.2770 | 931.0 | 719.0 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 18.85 | 104.80 | -0.50 | 1.54 | 0.3087 | 721.0 | 494.1 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 17.31 | 104.61 | -0.68 | 2.32 | 0.2829 | 789.0 | 662.4 | |
| 0.00 | 1.28 | 0.00 | 0.66 | 18.17 | 104.17 | -1.12 | 3.60 | 0.2978 | 759.0 | 551.5 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 18.76 | 102.42 | -2.87 | 8.83 | 0.3107 | 773.0 | 609.3 | |
| 0.00 | 1.20 | 0.00 | 0.61 | 15.22 | 102.14 | -3.16 | 12.19 | 0.2532 | 888.0 | 693.8 | |
| 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. | |