| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.88 | 0.00 | 13.17 | 7.08 | 207.28 | -30.78 | 87.84 | 0.5103 | 294.0 | 187.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.30 | 0.00 | 1.28 | 6.76 | 210.45 | -27.61 | 88.64 | 0.4623 | -747.0 | -670.3 | |
| 0.00 | 1.68 | 0.00 | 0.94 | 6.24 | 210.41 | -27.65 | 89.75 | 0.4632 | -773.0 | -634.7 | |
| 0.00 | 2.83 | 0.00 | 1.60 | 6.20 | 209.07 | -28.99 | 89.70 | 0.4838 | -800.0 | -619.8 | |
| 0.00 | 1.50 | 0.00 | 0.86 | 5.09 | 208.02 | -30.04 | 91.81 | 0.5009 | -651.0 | -409.1 | |
| 0.00 | 1.77 | 0.00 | 1.02 | 6.27 | 206.69 | -31.38 | 89.31 | 0.5196 | 621.0 | 552.2 | |
| 0.00 | 1.06 | 0.00 | 0.61 | 6.42 | 206.68 | -31.39 | 89.01 | 0.5197 | 724.0 | 630.6 | |
| 0.00 | 1.15 | 0.00 | 0.67 | 7.51 | 206.31 | -31.75 | 86.89 | 0.5245 | 802.0 | 654.1 | |
| 0.00 | 4.50 | 0.00 | 2.62 | 7.92 | 206.17 | -31.89 | 86.10 | 0.5266 | 827.0 | 715.2 | |
| 0.00 | 0.97 | 0.00 | 0.57 | 7.47 | 206.10 | -31.96 | 86.97 | 0.5277 | 763.0 | 648.0 | |
| 0.00 | 1.24 | 0.00 | 0.72 | 7.37 | 205.93 | -32.13 | 87.15 | 0.5302 | 606.0 | 442.7 | |
| 0.00 | 1.32 | 0.00 | 0.78 | 9.10 | 205.63 | -32.43 | 83.89 | 0.5347 | 732.0 | 614.2 | |
| 0.00 | 0.53 | 0.00 | 0.31 | 6.94 | 205.78 | -32.28 | 87.96 | 0.5326 | 621.0 | 555.3 | |
| 0.00 | 1.06 | 0.00 | 0.62 | 8.06 | 205.48 | -32.59 | 85.84 | 0.5368 | 714.0 | 565.8 | |
| 0.00 | 0.97 | 0.00 | 0.57 | 7.83 | 204.70 | -33.36 | 86.25 | 0.5481 | 677.0 | 538.2 | |
| 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. | |