| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.25 | 0.00 | 11.09 | -19.93 | 159.11 | -15.56 | 150.12 | 0.5078 | 607.9 | 417.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.27 | 0.00 | 0.71 | -20.42 | 165.38 | -9.30 | 161.31 | 0.4746 | 858.0 | 662.8 | |
| 0.00 | 1.90 | 0.00 | 1.10 | -21.95 | 160.11 | -14.56 | 153.58 | 0.5263 | 54.0 | 83.7 | |
| 0.00 | 1.90 | 0.00 | 1.10 | -21.20 | 159.99 | -14.69 | 152.69 | 0.5173 | 694.0 | 554.3 | |
| 0.00 | 1.54 | 0.00 | 0.88 | -19.94 | 159.75 | -14.93 | 151.07 | 0.5026 | 1004.0 | 759.8 | |
| 0.00 | 1.27 | 0.00 | 0.73 | -20.05 | 159.47 | -15.21 | 150.73 | 0.5061 | 792.0 | 576.4 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -17.60 | 159.63 | -15.05 | 148.32 | 0.4731 | 873.0 | 667.2 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -17.37 | 159.59 | -15.09 | 147.97 | 0.4705 | 819.0 | 638.5 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -20.81 | 159.12 | -15.56 | 150.95 | 0.5184 | 664.0 | 532.4 | |
| 0.00 | 2.17 | 0.00 | 1.22 | -17.27 | 159.43 | -15.25 | 147.59 | 0.4705 | 846.0 | 669.1 | |
| 0.00 | 0.72 | 0.00 | 0.41 | -17.04 | 159.32 | -15.36 | 147.13 | 0.4685 | 961.0 | 793.2 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -16.92 | 159.06 | -15.61 | 146.55 | 0.4691 | 771.0 | 684.2 | |
| 0.00 | 1.90 | 0.00 | 1.11 | -20.82 | 157.69 | -16.98 | 148.80 | 0.5292 | 643.0 | 537.0 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -20.86 | 157.49 | -17.19 | 148.54 | 0.5313 | 306.0 | 322.1 | |
| 0.00 | 2.17 | 0.00 | 1.30 | -21.93 | 154.51 | -20.17 | 145.56 | 0.5676 | -774.0 | -626.6 | |
| 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. | |