| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60 | 521 | 33 | 289 | -29.37 | 22.03 | 12.22 | 204.50 | 0.4480 | -1604.6 | -454.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 5 | 0 | 3 | -26.22 | 23.15 | 13.35 | 210.36 | 0.4115 | 633.0 | 379.8 | |
| 42 | 427 | 23 | 236 | -29.07 | 23.33 | 13.53 | 207.09 | 0.4508 | -1814.3 | -714.7 | |
| 18 | -2 | 10 | -2 | -29.34 | 22.60 | 12.79 | 205.56 | 0.4494 | -1855.4 | 999999 | |
| 0 | 3 | 0 | 2 | -27.10 | 22.07 | 12.26 | 207.22 | 0.4151 | 356.0 | 212.2 | |
| 0 | 11 | 0 | 6 | -30.19 | 19.91 | 10.10 | 200.00 | 0.4450 | 1050.0 | 790.7 | |
| 0 | 3 | 0 | 2 | -29.64 | 19.81 | 10.00 | 200.31 | 0.4366 | 825.0 | 689.0 | |
| 0 | 3 | 0 | 2 | -30.29 | 18.79 | 8.99 | 197.89 | 0.4408 | 599.0 | 532.5 | |
| 0 | 9 | 0 | 5 | -30.34 | 17.68 | 7.87 | 195.77 | 0.4366 | 691.0 | 642.3 | |
| 0 | 13 | 0 | 7 | -30.73 | 17.17 | 7.36 | 194.55 | 0.4403 | 1063.0 | 804.7 | |
| 0 | 6 | 0 | 3 | -30.86 | 16.68 | 6.88 | 193.55 | 0.4405 | 916.0 | 739.3 | |
| 0 | 4 | 0 | 2 | -30.31 | 16.60 | 6.79 | 193.74 | 0.4319 | 636.0 | 571.2 | |
| 0 | 5 | 0 | 3 | -30.83 | 16.19 | 6.38 | 192.63 | 0.4382 | 1026.0 | 833.6 | |
| 0 | 7 | 0 | 4 | -30.79 | 15.65 | 5.84 | 191.62 | 0.4358 | 1003.0 | 827.8 | |
| 0 | 4 | 0 | 2 | -30.96 | 15.03 | 5.22 | 190.34 | 0.4367 | 948.0 | 841.6 | |
| 0 | 7 | 0 | 4 | -30.97 | 14.62 | 4.82 | 189.56 | 0.4356 | 1220.0 | 1008.7 | |
| 0 | 9 | 0 | 5 | -31.06 | 14.13 | 4.33 | 188.57 | 0.4358 | 1003.0 | 688.2 | |
| 0 | 5 | 0 | 3 | -32.73 | 13.30 | 3.50 | 186.43 | 0.4600 | 610.0 | 446.9 | |
| 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. | |