| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.00 | 138.54 | 14.11 | 69.80 | -9.14 | 25.05 | 6.27 | 216.34 | 0.1820 | 763.6 | 448.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.99 | 29.35 | 1.00 | 14.82 | -8.90 | 26.12 | 7.34 | 222.08 | 0.1891 | 1092.7 | 497.9 | |
| 2.89 | -1.00 | 1.46 | -1.00 | -9.08 | 26.09 | 7.31 | 221.32 | 0.1912 | 1094.9 | 999999 | |
| 0.00 | 0.45 | 0.00 | 0.23 | -15.54 | 26.21 | 7.42 | 206.17 | 0.2834 | -206.0 | -194.8 | |
| 5.87 | 82.91 | 2.96 | 41.78 | -9.27 | 25.72 | 6.94 | 219.23 | 0.1895 | 999.5 | 503.6 | |
| 15.90 | -4.00 | 8.01 | -4.00 | -9.02 | 25.41 | 6.63 | 218.78 | 0.1828 | 1394.0 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.50 | -7.83 | 25.36 | 6.58 | 223.12 | 0.1668 | -574.0 | -396.2 | |
| 0.00 | 1.90 | 0.00 | 0.95 | -7.86 | 24.07 | 5.28 | 216.85 | 0.1528 | 904.0 | 704.3 | |
| 0.00 | 3.52 | 0.00 | 1.77 | -9.64 | 23.35 | 4.56 | 207.23 | 0.1722 | 1053.0 | 894.7 | |
| 0.00 | 5.51 | 0.00 | 2.77 | -10.04 | 23.20 | 4.41 | 205.44 | 0.1772 | 852.0 | 632.2 | |
| 1.35 | 5.78 | 0.68 | 2.91 | -9.85 | 22.85 | 4.07 | 204.13 | 0.1719 | 1109.2 | 848.6 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -9.36 | 22.29 | 3.51 | 202.26 | 0.1602 | 874.0 | 631.4 | |
| 0.00 | 1.45 | 0.00 | 0.72 | -9.08 | 20.54 | 1.75 | 191.94 | 0.1466 | -967.0 | -845.6 | |
| 0.00 | 3.52 | 0.00 | 1.76 | -8.41 | 19.89 | 1.10 | 188.28 | 0.1331 | -974.0 | -849.4 | |
| 0.00 | 1.99 | 0.00 | 1.00 | -9.30 | 19.74 | 0.95 | 186.39 | 0.1481 | -884.0 | -643.9 | |
| 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. | |