| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.12 | 0.00 | 10.70 | 6.15 | 261.97 | -25.27 | 74.78 | 0.4336 | 82.4 | 45.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.81 | 0.00 | 1.44 | 4.97 | 273.50 | -13.74 | 69.75 | 0.2534 | -655.0 | -537.5 | |
| 0.00 | 1.90 | 0.00 | 0.98 | 5.86 | 273.26 | -13.98 | 66.86 | 0.2626 | -618.0 | -490.2 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 4.36 | 273.04 | -14.20 | 72.59 | 0.2575 | -941.0 | -757.0 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 3.27 | 272.43 | -14.82 | 77.28 | 0.2629 | -817.0 | -612.8 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 3.97 | 271.44 | -15.81 | 75.59 | 0.2818 | -676.0 | -588.7 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 2.97 | 270.31 | -16.93 | 79.80 | 0.2969 | -859.0 | -638.8 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 8.12 | 260.37 | -26.88 | 72.42 | 0.4714 | 673.0 | 541.4 | |
| 0.00 | 0.54 | 0.00 | 0.31 | 7.97 | 259.96 | -27.28 | 72.96 | 0.4767 | 740.0 | 619.5 | |
| 0.00 | 0.81 | 0.00 | 0.46 | 5.39 | 258.87 | -28.37 | 78.70 | 0.4844 | 698.0 | 636.9 | |
| 0.00 | 1.99 | 0.00 | 1.16 | 5.86 | 256.24 | -31.01 | 78.68 | 0.5247 | 772.0 | 585.5 | |
| 0.00 | 1.36 | 0.00 | 0.81 | 7.39 | 254.35 | -32.89 | 76.51 | 0.5559 | 617.0 | 558.9 | |
| 0.00 | 1.09 | 0.00 | 0.67 | 5.19 | 250.52 | -36.72 | 81.31 | 0.6046 | 540.0 | 453.5 | |
| 0.00 | 1.18 | 0.00 | 0.74 | 8.91 | 249.87 | -37.37 | 75.48 | 0.6217 | 555.0 | 475.8 | |
| 0.00 | 0.54 | 0.00 | 0.35 | 9.65 | 248.64 | -38.60 | 74.72 | 0.6399 | 687.0 | 576.0 | |
| 0.00 | 1.45 | 0.00 | 0.94 | 9.53 | 248.30 | -38.95 | 75.01 | 0.6440 | 520.0 | 456.9 | |
| 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. | |