| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.36 | 246.80 | 46.00 | 258.85 | 11.89 | 262.38 | 59.20 | 287.55 | 0.8827 | -374.5 | -206.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.70 | 0.00 | 0.91 | 12.96 | 268.17 | 64.98 | 287.16 | 0.9259 | -237.0 | -224.9 | |
| 0.00 | 1.31 | 0.00 | 1.54 | 13.17 | 265.54 | 62.36 | 288.05 | 0.9090 | 294.0 | 236.8 | |
| 43.36 | 234.59 | 46.00 | 248.60 | 11.84 | 262.77 | 59.59 | 287.35 | 0.8862 | -591.3 | -232.7 | |
| 0.00 | 0.87 | 0.00 | 0.85 | 16.28 | 258.70 | 55.52 | 293.51 | 0.8649 | -356.0 | -306.3 | |
| 0.00 | 0.52 | 0.00 | 0.42 | 11.26 | 252.46 | 49.28 | 290.07 | 0.7936 | 360.0 | 324.7 | |
| 0.00 | 1.57 | 0.00 | 1.21 | 12.85 | 249.19 | 46.01 | 293.35 | 0.7663 | 531.0 | 393.1 | |
| 0.00 | 0.52 | 0.00 | 0.39 | 11.81 | 248.52 | 45.33 | 292.38 | 0.7552 | 487.0 | 446.8 | |
| 0.00 | 1.40 | 0.00 | 1.06 | 13.12 | 248.38 | 45.19 | 294.07 | 0.7591 | 567.0 | 508.8 | |
| 0.00 | 1.92 | 0.00 | 1.44 | 12.92 | 247.85 | 44.67 | 294.06 | 0.7527 | 651.0 | 570.6 | |
| 0.00 | 0.96 | 0.00 | 0.72 | 13.62 | 247.59 | 44.40 | 295.06 | 0.7530 | 404.0 | 380.3 | |
| 0.00 | 0.61 | 0.00 | 0.46 | 13.57 | 247.40 | 44.22 | 295.09 | 0.7509 | 581.0 | 567.6 | |
| 0.00 | 0.35 | 0.00 | 0.24 | 9.95 | 243.52 | 40.33 | 292.39 | 0.6918 | 508.0 | 495.8 | |
| 0.00 | 0.96 | 0.00 | 0.66 | 12.06 | 242.55 | 39.37 | 295.75 | 0.6910 | 644.0 | 560.6 | |
| 0.00 | 0.52 | 0.00 | 0.35 | 11.36 | 242.04 | 38.85 | 295.11 | 0.6815 | 672.0 | 585.3 | |
| 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. | |