| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r |
| 0 | 42 | 0 | 25 | 25.54 | 102.10 | 0.56 | 358.95 | 0.4815 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r |
| 0 | 7 | 0 | 4 | 26.08 | 104.46 | 2.92 | 354.66 | 0.4939 | |
| 0 | 6 | 0 | 3 | 25.49 | 102.87 | 1.33 | 357.51 | 0.4831 | |
| 0 | 1 | 0 | 1 | 25.83 | 102.49 | 0.94 | 358.25 | 0.4882 | |
| 0 | 3 | 0 | 2 | 25.63 | 102.28 | 0.75 | 358.61 | 0.4851 | |
| 0 | 2 | 0 | 1 | 26.02 | 102.00 | 0.46 | 359.16 | 0.4908 | |
| 0 | 7 | 0 | 4 | 26.05 | 101.73 | 0.18 | 359.66 | 0.4913 | |
| 0 | 5 | 0 | 3 | 26.07 | 101.02 | -0.52 | 0.95 | 0.4916 | |
| 0 | 5 | 0 | 3 | 23.50 | 102.07 | 0.53 | 358.92 | 0.4519 | |
| 0 | 0 | 0 | 0 | 26.50 | 100.66 | -0.88 | 1.59 | 0.4983 | |
| 0 | 3 | 0 | 2 | 25.12 | 100.55 | -0.99 | 1.89 | 0.4773 | |
| 0 | 2 | 0 | 1 | 25.96 | 99.90 | -1.64 | 3.02 | 0.4906 | |
| 0 | 1 | 0 | 1 | 25.29 | 100.12 | -1.43 | 2.70 | 0.4802 | |
| 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 | |