| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.47 | 55.51 | 9.66 | 27.52 | -6.49 | 147.22 | 0.94 | 211.52 | 0.0477 | 29.4 | 292.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.55 | 0.00 | 0.77 | -7.31 | 149.96 | 3.68 | 268.21 | 0.0640 | -515.0 | -314.2 | |
| 6.03 | 12.07 | 2.99 | 5.99 | -6.93 | 149.72 | 3.44 | 274.56 | 0.0600 | 978.3 | 815.2 | |
| 0.00 | 5.69 | 0.00 | 2.82 | -6.69 | 148.88 | 2.60 | 281.19 | 0.0461 | 1002.0 | 747.0 | |
| 3.53 | 6.55 | 1.75 | 3.25 | -7.05 | 148.76 | 2.48 | 273.59 | 0.0432 | 1114.6 | 845.1 | |
| 0.00 | 1.03 | 0.00 | 0.51 | -7.35 | 148.37 | 2.09 | 266.08 | 0.0364 | 969.0 | 782.0 | |
| 0.00 | 1.72 | 0.00 | 0.85 | -7.67 | 148.19 | 1.91 | 256.12 | 0.0342 | 1003.0 | 905.0 | |
| 0.00 | 2.24 | 0.00 | 1.11 | -7.56 | 148.19 | 1.91 | 259.55 | 0.0338 | 611.0 | 565.4 | |
| 0.00 | 2.07 | 0.00 | 1.03 | -6.49 | 148.04 | 1.76 | 292.36 | 0.0331 | 920.0 | 588.2 | |
| 0.00 | 1.90 | 0.00 | 0.94 | -5.24 | 147.26 | 0.98 | 333.56 | 0.0385 | -961.0 | -708.3 | |
| 0.00 | 0.86 | 0.00 | 0.43 | -5.15 | 147.05 | 0.77 | 339.46 | 0.0385 | -892.0 | -668.3 | |
| 0.00 | 2.33 | 0.00 | 1.15 | -5.96 | 146.85 | 0.56 | 335.89 | 0.0241 | 1073.0 | 842.5 | |
| 0.86 | 3.02 | 0.43 | 1.49 | -6.07 | 145.56 | -0.72 | 32.15 | 0.0236 | -1014.2 | -684.7 | |
| 0.00 | 1.29 | 0.00 | 0.64 | -5.24 | 144.16 | -2.12 | 46.94 | 0.0506 | -871.0 | -572.3 | |
| 9.05 | 13.19 | 4.49 | 6.54 | -5.82 | 143.38 | -2.90 | 64.44 | 0.0560 | -1148.4 | -819.0 | |
| 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. | |