| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.94 | 374.91 | 29.97 | 187.49 | -3.74 | 1.17 | -6.91 | 118.77 | 0.1376 | 1099.5 | 393.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.19 | 0.00 | 0.59 | -4.30 | 6.01 | -2.07 | 154.52 | 0.0840 | 1031.0 | 845.5 | |
| 32.74 | 363.91 | 16.36 | 181.95 | -3.83 | 1.50 | -6.58 | 120.43 | 0.1331 | 1504.1 | 407.6 | |
| 0.26 | -2.00 | 0.13 | -2.00 | -4.21 | 1.35 | -6.73 | 122.28 | 0.1389 | 981.3 | 999999 | |
| 26.94 | -2.00 | 13.48 | -2.00 | -3.53 | 0.85 | -7.23 | 116.26 | 0.1407 | 1435.5 | 999999 | |
| 0.00 | 0.77 | 0.00 | 0.39 | -5.96 | 0.40 | -7.68 | 128.11 | 0.1696 | 851.0 | 642.2 | |
| 0.00 | 0.60 | 0.00 | 0.30 | -4.74 | 0.36 | -7.72 | 121.82 | 0.1583 | 542.0 | 508.3 | |
| 0.00 | 0.77 | 0.00 | 0.39 | -5.04 | 359.96 | -8.11 | 122.11 | 0.1667 | 872.0 | 699.0 | |
| 0.00 | 1.11 | 0.00 | 0.56 | -6.08 | 359.56 | -8.52 | 125.80 | 0.1825 | -700.0 | -504.3 | |
| 0.00 | 0.85 | 0.00 | 0.43 | -5.69 | 359.47 | -8.60 | 123.78 | 0.1799 | -917.0 | -717.0 | |
| 0.00 | 1.62 | 0.00 | 0.82 | -5.12 | 358.28 | -9.79 | 117.91 | 0.1926 | -872.0 | -658.8 | |
| 0.00 | 1.88 | 0.00 | 0.94 | -3.26 | 358.25 | -9.83 | 108.58 | 0.1806 | 958.0 | 805.6 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -4.56 | 358.23 | -9.84 | 115.13 | 0.1891 | -996.0 | -803.2 | |
| 0.00 | 1.19 | 0.00 | 0.60 | -4.89 | 358.11 | -9.97 | 116.39 | 0.1935 | -789.0 | -518.4 | |
| 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. | |