| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.92 | 0.00 | 9.89 | 4.44 | 81.79 | 41.29 | 276.35 | 0.6637 | 213.6 | 196.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.51 | 0.00 | 0.37 | 7.70 | 86.39 | 45.89 | 280.35 | 0.7256 | -494.0 | -414.0 | |
| 0.00 | 0.85 | 0.00 | 0.60 | 5.02 | 85.53 | 45.02 | 276.76 | 0.7120 | -539.0 | -491.3 | |
| 0.00 | 1.62 | 0.00 | 1.14 | 4.93 | 85.39 | 44.89 | 276.65 | 0.7103 | -572.0 | -403.4 | |
| 0.00 | 0.85 | 0.00 | 0.59 | 5.29 | 85.01 | 44.50 | 277.20 | 0.7059 | -623.0 | -589.0 | |
| 0.00 | 0.68 | 0.00 | 0.46 | 4.03 | 82.70 | 42.19 | 275.62 | 0.6756 | 517.0 | 414.4 | |
| 0.00 | 1.54 | 0.00 | 1.02 | 2.99 | 82.44 | 41.94 | 274.11 | 0.6714 | 533.0 | 421.7 | |
| 0.00 | 1.19 | 0.00 | 0.80 | 4.77 | 82.51 | 42.01 | 276.74 | 0.6739 | 450.0 | 386.9 | |
| 0.00 | 0.51 | 0.00 | 0.34 | 2.99 | 82.08 | 41.58 | 274.14 | 0.6668 | 575.0 | 541.8 | |
| 0.00 | 1.37 | 0.00 | 0.90 | 4.59 | 81.86 | 41.36 | 276.56 | 0.6653 | 544.0 | 477.2 | |
| 0.00 | 0.51 | 0.00 | 0.34 | 3.03 | 81.76 | 41.26 | 274.21 | 0.6627 | 645.0 | 587.2 | |
| 0.00 | 1.19 | 0.00 | 0.77 | 1.35 | 80.38 | 39.88 | 271.70 | 0.6436 | 542.0 | 451.9 | |
| 0.00 | 0.77 | 0.00 | 0.50 | 7.13 | 80.52 | 40.01 | 280.62 | 0.6515 | -520.0 | -360.7 | |
| 0.00 | 1.11 | 0.00 | 0.69 | 3.67 | 77.25 | 36.75 | 275.67 | 0.6023 | 785.0 | 635.1 | |
| 0.00 | 1.45 | 0.00 | 0.90 | 3.70 | 77.07 | 36.56 | 275.75 | 0.5998 | 757.0 | 673.6 | |
| 0.00 | 0.77 | 0.00 | 0.47 | 8.37 | 76.11 | 35.61 | 283.74 | 0.5952 | 604.0 | 525.6 | |
| 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. | |