| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.32 | 68.20 | 3.17 | 34.34 | -11.23 | 13.41 | -9.15 | 114.70 | 0.1724 | 583.5 | 112.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.30 | 0.00 | 0.65 | -10.81 | 18.07 | -4.50 | 129.12 | 0.0997 | 859.0 | 698.4 | |
| 0.00 | 5.03 | 0.00 | 2.50 | -9.01 | 17.46 | -5.11 | 109.70 | 0.0938 | 1001.0 | 857.3 | |
| 0.95 | 2.17 | 0.47 | 1.08 | -10.05 | 16.99 | -5.58 | 117.41 | 0.1083 | 1164.1 | 909.4 | |
| 0.00 | 2.25 | 0.00 | 1.12 | -10.31 | 16.62 | -5.95 | 118.04 | 0.1160 | 1083.0 | 837.7 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -11.13 | 15.74 | -6.82 | 120.57 | 0.1359 | 921.0 | 692.1 | |
| 0.00 | 1.82 | 0.00 | 0.91 | -11.54 | 15.30 | -7.26 | 121.58 | 0.1460 | 783.0 | 675.8 | |
| 2.25 | 9.10 | 1.13 | 4.55 | -11.06 | 15.04 | -7.52 | 117.82 | 0.1459 | 1146.2 | 839.1 | |
| 2.08 | 9.79 | 1.04 | 4.90 | -10.16 | 14.70 | -7.86 | 111.18 | 0.1451 | 1239.8 | 915.1 | |
| 0.00 | 2.60 | 0.00 | 1.31 | -11.58 | 14.20 | -8.36 | 118.42 | 0.1628 | 797.0 | 609.8 | |
| 0.00 | 1.82 | 0.00 | 0.91 | -11.11 | 14.15 | -8.41 | 115.61 | 0.1599 | 991.0 | 783.8 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -10.75 | 14.16 | -8.40 | 113.55 | 0.1573 | 755.0 | 589.2 | |
| 0.00 | 0.87 | 0.00 | 0.44 | -11.16 | 13.84 | -8.72 | 115.15 | 0.1650 | 702.0 | 499.4 | |
| 0.00 | 0.78 | 0.00 | 0.39 | -7.22 | 13.40 | -9.16 | 90.45 | 0.1587 | 748.0 | 606.9 | |
| 0.00 | 1.65 | 0.00 | 0.83 | -11.29 | 12.86 | -9.71 | 113.65 | 0.1813 | -771.0 | -547.5 | |
| 0.00 | 1.04 | 0.00 | 0.53 | -11.86 | 10.67 | -11.89 | 112.43 | 0.2192 | -832.0 | -651.2 | |
| 1.04 | 24.09 | 0.53 | 12.25 | -12.37 | 10.58 | -11.98 | 114.43 | 0.2237 | -1095.3 | -764.2 | |
| 0.00 | 1.73 | 0.00 | 0.88 | -12.44 | 9.92 | -12.64 | 113.67 | 0.2344 | -734.0 | -583.5 | |
| 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. | |