| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 96 | 583 | 100 | 606 | 4.45 | 72.18 | 60.71 | 278.25 | 0.8789 | -64.3 | -38.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18 | 138 | 22 | 170 | 4.11 | 77.33 | 65.86 | 276.98 | 0.9187 | 303.4 | 44.5 | |
| 5 | -1 | 7 | -1 | 4.09 | 76.67 | 65.20 | 277.06 | 0.9142 | 754.2 | 999999 | |
| 0 | 12 | 0 | 14 | 3.90 | 75.91 | 64.44 | 276.98 | 0.9086 | 575.0 | 513.1 | |
| 2 | 60 | 2 | 66 | 3.37 | 75.13 | 63.66 | 276.51 | 0.9023 | 395.8 | 582.4 | |
| 12 | -4 | 13 | -4 | 3.78 | 74.07 | 62.60 | 277.13 | 0.8947 | 832.3 | 999999 | |
| -5 | -4 | -5 | -4 | 4.15 | 73.95 | 62.48 | 277.57 | 0.8942 | 999999 | 999999 | |
| 5 | 31 | 6 | 33 | 4.69 | 72.55 | 61.08 | 278.40 | 0.8838 | 940.9 | 621.6 | |
| 4 | -7 | 4 | -7 | 4.95 | 72.43 | 60.96 | 278.72 | 0.8832 | 857.5 | 999999 | |
| 0 | 2 | 0 | 2 | 2.93 | 71.01 | 59.54 | 276.67 | 0.8688 | -122.0 | -154.5 | |
| 0 | 5 | 0 | 5 | 5.42 | 70.64 | 59.17 | 279.58 | 0.8690 | 369.0 | 467.3 | |
| 12 | 250 | 11 | 237 | 3.33 | 69.85 | 58.38 | 277.33 | 0.8592 | -623.7 | -280.4 | |
| 12 | -11 | 11 | -11 | 4.22 | 69.28 | 57.81 | 278.46 | 0.8554 | -876.9 | 999999 | |
| 8 | -11 | 8 | -11 | 4.68 | 68.76 | 57.29 | 279.09 | 0.8514 | -950.6 | 999999 | |
| 5 | -11 | 4 | -11 | 5.42 | 68.30 | 56.82 | 280.04 | 0.8484 | -679.4 | 999999 | |
| 0 | 2 | 0 | 2 | 6.05 | 68.39 | 56.92 | 280.76 | 0.8503 | -357.0 | -324.2 | |
| 13 | 83 | 12 | 77 | 6.44 | 67.97 | 56.49 | 281.31 | 0.8471 | -1032.6 | -415.1 | |
| 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. | |