| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.16 | 40.36 | 4.86 | 21.77 | 5.44 | 71.46 | -23.14 | 85.60 | 0.3936 | -186.5 | -278.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.85 | 21.44 | 1.51 | 11.37 | 5.84 | 73.74 | -20.86 | 84.32 | 0.3576 | -1304.7 | -853.3 | |
| 4.15 | -1.00 | 2.20 | -1.00 | 5.89 | 73.54 | -21.06 | 84.20 | 0.3608 | -975.1 | 999999 | |
| 2.16 | -1.00 | 1.15 | -1.00 | 5.68 | 73.52 | -21.08 | 84.79 | 0.3610 | -1093.5 | 999999 | |
| 0.00 | 1.64 | 0.00 | 0.87 | 5.50 | 73.36 | -21.24 | 85.31 | 0.3633 | -695.0 | -627.2 | |
| 0.00 | 0.61 | 0.00 | 0.32 | 5.11 | 73.31 | -21.29 | 86.39 | 0.3639 | -701.0 | -602.3 | |
| 0.00 | 1.64 | 0.00 | 0.87 | 5.74 | 73.26 | -21.34 | 84.68 | 0.3653 | -697.0 | -594.2 | |
| 0.00 | 0.95 | 0.00 | 0.51 | 5.43 | 72.82 | -21.78 | 85.58 | 0.3721 | -731.0 | -603.3 | |
| 0.00 | 4.06 | 0.00 | 2.18 | 3.44 | 71.91 | -22.69 | 90.85 | 0.3867 | -726.0 | -513.0 | |
| 0.00 | 0.95 | 0.00 | 0.53 | 6.03 | 67.70 | -26.90 | 84.72 | 0.4537 | 770.0 | 542.7 | |
| 0.00 | 0.95 | 0.00 | 0.53 | 6.05 | 67.37 | -27.23 | 84.71 | 0.4589 | 765.0 | 557.5 | |
| 0.00 | 1.12 | 0.00 | 0.63 | 5.71 | 66.95 | -27.65 | 85.49 | 0.4652 | 904.0 | 802.7 | |
| 0.00 | 1.12 | 0.00 | 0.63 | 4.65 | 66.39 | -28.21 | 87.78 | 0.4735 | 925.0 | 786.0 | |
| 0.00 | 1.99 | 0.00 | 1.12 | 5.09 | 66.16 | -28.44 | 86.85 | 0.4770 | 789.0 | 571.3 | |
| 0.00 | 1.90 | 0.00 | 1.07 | 4.49 | 66.19 | -28.41 | 88.11 | 0.4765 | 894.0 | 709.2 | |
| 0.00 | 1.99 | 0.00 | 1.14 | 6.22 | 64.35 | -30.25 | 84.65 | 0.5050 | 731.0 | 485.1 | |
| 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. | |