| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.99 | 0.00 | 8.58 | 12.82 | 61.09 | -6.54 | 161.03 | 0.1837 | 53.5 | 36.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.40 | 0.00 | 0.71 | 14.94 | 74.08 | 6.45 | 324.42 | 0.1874 | -779.0 | -617.9 | |
| 0.00 | 0.70 | 0.00 | 0.35 | 14.50 | 67.32 | -0.31 | 2.12 | 0.1443 | -783.0 | -602.5 | |
| 0.00 | 1.05 | 0.00 | 0.53 | 14.20 | 66.85 | -0.78 | 5.44 | 0.1396 | -730.0 | -613.8 | |
| 0.00 | 1.31 | 0.00 | 0.65 | 8.07 | 66.08 | -1.56 | 40.22 | 0.0418 | 682.0 | 503.5 | |
| 0.00 | 1.23 | 0.00 | 0.61 | 12.36 | 65.14 | -2.49 | 21.74 | 0.1151 | -921.0 | -733.1 | |
| 0.00 | 1.49 | 0.00 | 0.75 | 15.85 | 63.30 | -4.33 | 23.50 | 0.1830 | -832.0 | -712.5 | |
| 0.00 | 1.31 | 0.00 | 0.65 | 10.51 | 63.26 | -4.37 | 45.08 | 0.1062 | -881.0 | -647.1 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 10.57 | 62.74 | -4.89 | 47.88 | 0.1134 | -952.0 | -753.7 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 13.83 | 58.40 | -9.23 | 49.45 | 0.2059 | 802.0 | 594.7 | |
| 0.00 | 1.40 | 0.00 | 0.71 | 13.45 | 57.20 | -10.43 | 54.20 | 0.2181 | 1015.0 | 853.7 | |
| 0.00 | 1.05 | 0.00 | 0.53 | 12.78 | 56.98 | -10.65 | 57.35 | 0.2151 | 953.0 | 652.5 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 9.99 | 54.56 | -13.07 | 73.01 | 0.2339 | 702.0 | 586.5 | |
| 0.00 | 1.14 | 0.00 | 0.58 | 12.41 | 53.60 | -14.03 | 65.00 | 0.2624 | 954.0 | 744.2 | |
| 0.00 | 1.23 | 0.00 | 0.63 | 13.91 | 53.33 | -14.31 | 60.36 | 0.2772 | 750.0 | 680.9 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 14.44 | 49.69 | -17.94 | 63.69 | 0.3343 | 823.0 | 633.7 | |
| 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. | |