| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.79 | 204.17 | 19.03 | 102.79 | 13.61 | 291.51 | 8.12 | 309.54 | 0.1794 | -572.3 | -413.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.90 | 0.00 | 0.46 | 17.86 | 293.19 | 9.80 | 319.06 | 0.2483 | 833.0 | 537.4 | |
| 9.31 | 191.55 | 4.69 | 96.44 | 13.20 | 291.86 | 8.48 | 306.44 | 0.1792 | -1223.7 | -506.6 | |
| 4.75 | -2.00 | 2.39 | -2.00 | 14.08 | 291.87 | 8.48 | 310.30 | 0.1883 | -1247.7 | 999999 | |
| 21.67 | -2.00 | 10.91 | -2.00 | 13.51 | 291.62 | 8.23 | 308.61 | 0.1790 | -1320.0 | 999999 | |
| 2.06 | -2.00 | 1.04 | -2.00 | 13.97 | 291.55 | 8.16 | 310.87 | 0.1829 | -1097.3 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.31 | 11.91 | 290.57 | 7.18 | 304.22 | 0.1487 | 804.0 | 645.0 | |
| 0.00 | 1.34 | 0.00 | 0.67 | 12.16 | 290.18 | 6.79 | 307.13 | 0.1455 | 915.0 | 737.8 | |
| 0.00 | 1.16 | 0.00 | 0.58 | 10.93 | 289.56 | 6.17 | 301.96 | 0.1249 | 1029.0 | 824.9 | |
| 0.00 | 1.43 | 0.00 | 0.72 | 15.14 | 288.03 | 4.64 | 330.64 | 0.1598 | 848.0 | 657.2 | |
| 0.00 | 3.76 | 0.00 | 1.89 | 15.61 | 287.63 | 4.24 | 334.11 | 0.1637 | 1021.0 | 752.3 | |
| 0.00 | 1.25 | 0.00 | 0.63 | 15.64 | 287.19 | 3.80 | 336.57 | 0.1611 | 862.0 | 711.3 | |
| 0.00 | 1.16 | 0.00 | 0.59 | 16.22 | 286.91 | 3.52 | 339.42 | 0.1686 | 821.0 | 671.8 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 16.56 | 286.79 | 3.40 | 340.75 | 0.1734 | 1088.0 | 921.4 | |
| 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. | |