| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.90 | 36.28 | 1.52 | 18.82 | 13.03 | 92.41 | -15.35 | 65.07 | 0.2842 | 105.1 | 31.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.67 | 0.00 | 0.84 | 10.70 | 99.92 | -7.85 | 60.65 | 0.1546 | -859.0 | -703.2 | |
| 0.00 | 2.19 | 0.00 | 1.10 | 10.43 | 99.55 | -8.21 | 63.27 | 0.1580 | -892.0 | -687.3 | |
| 0.00 | 0.97 | 0.00 | 0.48 | 10.06 | 99.41 | -8.36 | 65.74 | 0.1577 | -887.0 | -573.4 | |
| 0.00 | 1.32 | 0.00 | 0.66 | 10.77 | 98.80 | -8.96 | 63.28 | 0.1721 | -787.0 | -669.5 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 13.42 | 98.62 | -9.14 | 51.47 | 0.1984 | -824.0 | -670.2 | |
| 0.00 | 1.14 | 0.00 | 0.57 | 10.58 | 98.19 | -9.57 | 65.67 | 0.1802 | -787.0 | -708.3 | |
| 0.00 | 2.28 | 0.00 | 1.15 | 10.69 | 97.60 | -10.16 | 66.33 | 0.1902 | -1104.0 | -851.4 | |
| 0.00 | 5.97 | 0.00 | 3.01 | 10.26 | 97.15 | -10.61 | 69.24 | 0.1947 | -807.0 | -785.6 | |
| 0.00 | 0.97 | 0.00 | 0.50 | 17.18 | 92.98 | -14.79 | 52.06 | 0.3105 | 797.0 | 664.8 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 16.94 | 89.90 | -17.87 | 57.43 | 0.3498 | 765.0 | 630.2 | |
| 2.90 | 7.64 | 1.52 | 4.01 | 13.50 | 89.45 | -18.32 | 67.20 | 0.3330 | 1139.0 | 926.4 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 15.46 | 88.29 | -19.47 | 63.10 | 0.3618 | 807.0 | 631.9 | |
| 0.00 | 1.32 | 0.00 | 0.70 | 12.64 | 87.46 | -20.30 | 71.25 | 0.3591 | 733.0 | 596.7 | |
| 0.00 | 2.37 | 0.00 | 1.27 | 14.67 | 86.62 | -21.15 | 66.67 | 0.3817 | 929.0 | 818.0 | |
| 0.00 | 0.97 | 0.00 | 0.52 | 14.30 | 86.59 | -21.18 | 67.61 | 0.3802 | 817.0 | 642.1 | |
| 0.00 | 1.93 | 0.00 | 1.05 | 15.83 | 84.48 | -23.29 | 65.67 | 0.4192 | 647.0 | 641.5 | |
| 0.00 | 1.23 | 0.00 | 0.68 | 20.27 | 83.67 | -24.09 | 57.04 | 0.4583 | 906.0 | 716.7 | |
| 0.00 | 0.97 | 0.00 | 0.53 | 16.14 | 83.99 | -23.77 | 65.34 | 0.4278 | 762.0 | 597.0 | |
| 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. | |