| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.94 | 24.96 | 6.10 | 17.65 | -14.92 | 249.11 | -40.09 | 119.20 | 0.7140 | 186.4 | -67.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.02 | 11.77 | 4.10 | 8.03 | -15.29 | 251.68 | -37.52 | 121.19 | 0.6890 | 922.3 | 557.8 | |
| 0.00 | 0.53 | 0.00 | 0.36 | -13.89 | 251.97 | -37.24 | 119.55 | 0.6775 | 753.0 | 650.0 | |
| 2.92 | -1.00 | 2.00 | -1.00 | -15.53 | 251.59 | -37.61 | 121.43 | 0.6914 | 692.6 | 999999 | |
| 0.00 | 1.68 | 0.00 | 1.13 | -13.87 | 251.77 | -37.43 | 119.40 | 0.6796 | 688.0 | 605.6 | |
| 0.00 | 0.89 | 0.00 | 0.60 | -13.75 | 251.64 | -37.56 | 119.16 | 0.6804 | 634.0 | 556.6 | |
| 0.00 | 0.80 | 0.00 | 0.57 | -13.89 | 247.20 | -42.00 | 116.70 | 0.7294 | -736.0 | -636.7 | |
| 0.00 | 0.80 | 0.00 | 0.58 | -13.94 | 246.98 | -42.22 | 116.64 | 0.7320 | -652.0 | -560.7 | |
| 0.00 | 2.12 | 0.00 | 1.57 | -15.47 | 246.35 | -42.85 | 118.20 | 0.7460 | -586.0 | -530.6 | |
| 0.00 | 0.35 | 0.00 | 0.26 | -13.96 | 246.68 | -42.52 | 116.51 | 0.7353 | -636.0 | -622.8 | |
| 0.00 | 1.15 | 0.00 | 0.85 | -14.18 | 245.99 | -43.21 | 116.42 | 0.7436 | -695.0 | -584.0 | |
| 0.00 | 1.68 | 0.00 | 1.26 | -14.82 | 245.66 | -43.54 | 117.04 | 0.7500 | -749.0 | -648.6 | |
| 0.00 | 1.42 | 0.00 | 1.07 | -15.02 | 244.92 | -44.29 | 116.89 | 0.7584 | -654.0 | -563.4 | |
| 0.00 | 0.97 | 0.00 | 0.75 | -14.91 | 244.28 | -44.92 | 116.44 | 0.7643 | 421.0 | 337.1 | |
| 0.00 | 0.80 | 0.00 | 0.62 | -14.66 | 243.51 | -45.69 | 115.76 | 0.7710 | 420.0 | 394.0 | |
| 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. | |