| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 95 | 767 | 48 | 398 | 2.69 | 271.90 | -16.08 | 94.95 | 0.2791 | 1801.4 | 692.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34 | 696 | 17 | 358 | 2.24 | 272.97 | -15.01 | 96.95 | 0.2618 | 2217.5 | 731.3 | |
| 15 | -1 | 8 | -1 | 2.19 | 272.46 | -15.52 | 96.87 | 0.2706 | 1664.4 | 999999 | |
| 12 | -1 | 6 | -1 | 3.38 | 272.08 | -15.90 | 92.38 | 0.2750 | 1660.8 | 999999 | |
| 0 | 6 | 0 | 3 | 0.80 | 271.95 | -16.04 | 101.54 | 0.2832 | 832.0 | 684.0 | |
| 6 | -1 | 3 | -1 | 3.33 | 271.60 | -16.38 | 92.45 | 0.2831 | 1348.2 | 999999 | |
| 28 | -1 | 14 | -1 | 2.87 | 271.57 | -16.42 | 94.08 | 0.2843 | 1790.2 | 999999 | |
| 0 | 7 | 0 | 4 | 0.48 | 271.59 | -16.39 | 102.34 | 0.2902 | 557.0 | 387.4 | |
| 0 | 5 | 0 | 3 | 4.36 | 271.01 | -16.97 | 88.80 | 0.2924 | 627.0 | 500.6 | |
| 0 | 8 | 0 | 4 | 4.01 | 270.74 | -17.24 | 89.99 | 0.2970 | 51.0 | 117.1 | |
| 0 | 9 | 0 | 5 | 4.40 | 269.43 | -18.55 | 88.66 | 0.3187 | 574.0 | 417.0 | |
| 0 | 6 | 0 | 3 | 2.84 | 267.17 | -20.81 | 93.03 | 0.3569 | 835.0 | 722.5 | |
| 0 | 5 | 0 | 3 | 3.92 | 266.98 | -21.00 | 89.99 | 0.3591 | 498.0 | 388.5 | |
| 0 | 13 | 0 | 7 | 3.26 | 266.96 | -21.02 | 91.82 | 0.3600 | 682.0 | 666.1 | |
| 0 | 3 | 0 | 2 | 2.29 | 266.73 | -21.25 | 94.45 | 0.3649 | 728.0 | 730.1 | |
| 0 | 3 | 0 | 2 | 4.71 | 266.46 | -21.52 | 87.79 | 0.3675 | -904.0 | -780.8 | |
| 0 | 3 | 0 | 2 | 4.55 | 264.96 | -23.02 | 88.22 | 0.3917 | -414.0 | -314.1 | |
| 0 | 3 | 0 | 2 | 4.82 | 263.60 | -24.38 | 87.56 | 0.4135 | -550.0 | -514.0 | |
| 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. | |