| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.69 | 109.79 | 11.19 | 62.72 | 16.35 | 41.24 | -24.69 | 53.68 | 0.4984 | -313.9 | -168.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.81 | 0.00 | 0.47 | 19.59 | 42.99 | -22.94 | 46.64 | 0.5070 | 751.0 | 564.0 | |
| 0.00 | 1.63 | 0.00 | 0.93 | 19.40 | 42.77 | -23.15 | 47.19 | 0.5075 | 737.0 | 586.0 | |
| 16.07 | 76.12 | 9.07 | 42.95 | 16.19 | 42.59 | -23.34 | 52.64 | 0.4805 | -1170.7 | -388.1 | |
| 1.54 | 2.35 | 0.87 | 1.33 | 15.25 | 41.40 | -24.53 | 55.58 | 0.4876 | -907.1 | -823.0 | |
| 0.00 | 0.54 | 0.00 | 0.31 | 15.38 | 41.24 | -24.69 | 55.51 | 0.4905 | -545.0 | -443.8 | |
| 0.00 | 1.17 | 0.00 | 0.67 | 16.20 | 40.85 | -25.07 | 54.48 | 0.5020 | -586.0 | -541.2 | |
| 0.36 | 2.71 | 0.21 | 1.55 | 15.89 | 40.79 | -25.14 | 55.09 | 0.5002 | -988.0 | -783.2 | |
| 0.00 | 2.62 | 0.00 | 1.50 | 15.73 | 40.64 | -25.29 | 55.51 | 0.5009 | -812.0 | -709.6 | |
| 0.00 | 1.08 | 0.00 | 0.62 | 15.89 | 40.44 | -25.49 | 55.43 | 0.5046 | -630.0 | -518.5 | |
| 0.00 | 1.17 | 0.00 | 0.67 | 15.32 | 39.75 | -26.18 | 57.07 | 0.5090 | -687.0 | -514.0 | |
| 0.00 | 0.90 | 0.00 | 0.52 | 15.17 | 38.64 | -27.29 | 58.33 | 0.5220 | 746.0 | 614.2 | |
| 0.00 | 7.22 | 0.00 | 4.27 | 17.31 | 37.74 | -28.19 | 55.63 | 0.5486 | 915.0 | 748.8 | |
| 0.00 | 1.35 | 0.00 | 0.82 | 17.19 | 35.71 | -30.22 | 57.49 | 0.5723 | 850.0 | 672.8 | |
| 0.00 | 1.99 | 0.00 | 1.20 | 16.87 | 35.69 | -30.23 | 58.00 | 0.5703 | 853.0 | 765.9 | |
| 0.00 | 1.17 | 0.00 | 0.70 | 15.92 | 35.64 | -30.29 | 59.54 | 0.5648 | 802.0 | 584.5 | |
| 0.00 | 1.54 | 0.00 | 0.93 | 16.75 | 35.38 | -30.54 | 58.43 | 0.5733 | 820.0 | 670.8 | |
| 1.72 | 3.70 | 1.04 | 2.24 | 17.01 | 35.08 | -30.85 | 58.27 | 0.5787 | 590.5 | 639.2 | |
| 0.00 | 1.72 | 0.00 | 1.04 | 17.23 | 34.96 | -30.96 | 58.01 | 0.5816 | 553.0 | 487.7 | |
| 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. | |