| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.94 | 108.36 | 27.40 | 263.88 | 9.10 | 172.40 | -78.88 | 81.89 | 0.9790 | 68.1 | 60.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.09 | 0.00 | 1.56 | 7.79 | 180.95 | -70.33 | 83.84 | 0.9399 | -229.0 | -258.2 | |
| 0.00 | 3.44 | 0.00 | 5.67 | 10.51 | 178.01 | -73.27 | 80.80 | 0.9552 | -532.0 | -408.3 | |
| 3.89 | 10.32 | 6.40 | 16.90 | 10.20 | 178.09 | -73.19 | 81.12 | 0.9549 | -572.1 | -336.1 | |
| 0.00 | 2.35 | 0.00 | 4.58 | 10.09 | 175.32 | -75.96 | 81.08 | 0.9679 | 418.0 | 389.0 | |
| 0.00 | 0.81 | 0.00 | 1.60 | 10.35 | 175.13 | -76.15 | 80.80 | 0.9687 | 351.0 | 346.4 | |
| 0.00 | 1.27 | 0.00 | 2.77 | 10.99 | 173.48 | -77.80 | 80.04 | 0.9752 | 197.0 | 264.4 | |
| 0.00 | 0.81 | 0.00 | 1.87 | 11.09 | 172.92 | -78.36 | 79.90 | 0.9772 | 137.0 | 160.6 | |
| 0.00 | 1.18 | 0.00 | 2.91 | 11.37 | 171.98 | -79.30 | 79.56 | 0.9804 | 299.0 | 306.1 | |
| 0.00 | 6.07 | 0.00 | 13.15 | 9.22 | 173.75 | -77.53 | 81.87 | 0.9746 | 538.0 | 456.5 | |
| 0.00 | 1.18 | 0.00 | 2.71 | 8.78 | 173.03 | -78.25 | 82.28 | 0.9774 | 424.0 | 441.2 | |
| 0.00 | 0.63 | 0.00 | 1.65 | 10.17 | 171.48 | -79.80 | 80.74 | 0.9823 | 317.0 | 320.6 | |
| 1.45 | 35.12 | 3.57 | 90.29 | 8.66 | 172.16 | -79.12 | 82.33 | 0.9805 | 396.5 | 128.2 | |
| 4.16 | 44.09 | 10.88 | 118.22 | 9.21 | 171.51 | -79.77 | 81.72 | 0.9825 | 284.4 | -16.1 | |
| 2.44 | -12.00 | 6.55 | -12.00 | 8.29 | 171.24 | -80.04 | 82.64 | 0.9836 | -33.9 | 999999 | |
| 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. | |