| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9 | 131 | 4 | 63 | 9.01 | 342.19 | 10.01 | 282.57 | 0.1794 | 125.9 | -142.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 3 | 0 | 1 | 6.10 | 347.42 | 15.23 | 266.56 | 0.2629 | -629.0 | -644.1 | |
| 0 | 11 | 0 | 5 | 6.95 | 345.24 | 13.06 | 269.49 | 0.2253 | -854.0 | -745.2 | |
| 0 | 7 | 0 | 3 | 6.73 | 344.79 | 12.61 | 268.38 | 0.2179 | -855.0 | -847.6 | |
| 0 | 5 | 0 | 2 | 7.13 | 344.48 | 12.30 | 270.20 | 0.2123 | -1032.0 | -909.6 | |
| 0 | 6 | 0 | 3 | 7.22 | 344.08 | 11.89 | 270.59 | 0.2054 | -860.0 | -725.7 | |
| 0 | 7 | 0 | 4 | 6.64 | 343.54 | 11.35 | 267.61 | 0.1966 | -865.0 | -700.3 | |
| 0 | 4 | 0 | 2 | 6.26 | 343.33 | 11.15 | 265.53 | 0.1936 | -893.0 | -746.1 | |
| 0 | 4 | 0 | 2 | 5.98 | 343.28 | 11.10 | 264.09 | 0.1934 | -762.0 | -689.8 | |
| 0 | 4 | 0 | 2 | 9.56 | 342.93 | 10.75 | 283.00 | 0.1896 | 761.0 | 569.7 | |
| 4 | 14 | 2 | 7 | 8.82 | 342.87 | 10.69 | 279.13 | 0.1865 | 1007.2 | 699.7 | |
| 0 | 12 | 0 | 6 | 9.69 | 342.53 | 10.35 | 284.11 | 0.1834 | 1201.0 | 923.5 | |
| 0 | 9 | 0 | 4 | 11.68 | 341.30 | 9.12 | 296.89 | 0.1748 | 1019.0 | 762.2 | |
| 0 | 6 | 0 | 3 | 10.04 | 340.85 | 8.66 | 288.62 | 0.1573 | 987.0 | 837.7 | |
| 2 | 8 | 1 | 4 | 10.51 | 340.58 | 8.40 | 292.06 | 0.1556 | 700.8 | 410.4 | |
| 3 | 10 | 1 | 5 | 10.84 | 339.66 | 7.48 | 296.48 | 0.1435 | -902.0 | -683.1 | |
| 0 | 10 | 0 | 5 | 10.57 | 339.25 | 7.07 | 295.95 | 0.1352 | -951.0 | -715.3 | |
| 0 | 11 | 0 | 5 | 10.93 | 339.18 | 7.00 | 298.53 | 0.1368 | -1054.0 | -834.8 | |
| 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. | |