| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53 | 370 | 28 | 194 | -12.73 | 177.07 | -9.01 | 151.02 | 0.3182 | 1415.7 | 556.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 2 | -16.62 | 179.52 | -6.56 | 162.21 | 0.3599 | -655.0 | -594.7 | |
| 0 | 4 | 0 | 2 | -16.38 | 179.05 | -7.04 | 160.78 | 0.3587 | -762.0 | -566.3 | |
| 0 | 6 | 0 | 3 | -12.10 | 178.75 | -7.34 | 154.86 | 0.2953 | 308.0 | 253.7 | |
| 19 | 316 | 10 | 165 | -13.35 | 177.79 | -8.29 | 153.94 | 0.3208 | 1287.0 | 742.5 | |
| 21 | -4 | 11 | -4 | -12.35 | 177.47 | -8.62 | 151.55 | 0.3086 | 1940.7 | 999999 | |
| 8 | -4 | 4 | -4 | -12.56 | 176.86 | -9.22 | 150.23 | 0.3164 | 1690.9 | 999999 | |
| 5 | -4 | 3 | -4 | -13.04 | 176.85 | -9.24 | 150.94 | 0.3235 | 1178.4 | 999999 | |
| 0 | 3 | 0 | 2 | -19.25 | 175.89 | -10.20 | 156.45 | 0.4201 | -679.0 | -541.4 | |
| 0 | 5 | 0 | 3 | -9.33 | 174.95 | -11.14 | 138.90 | 0.2912 | -696.0 | -603.9 | |
| 0 | 3 | 0 | 2 | -10.63 | 174.66 | -11.42 | 141.03 | 0.3109 | -755.0 | -545.8 | |
| 0 | 6 | 0 | 3 | -9.10 | 174.56 | -11.53 | 137.38 | 0.2927 | -918.0 | -768.3 | |
| 0 | 4 | 0 | 2 | -14.60 | 173.91 | -12.17 | 146.39 | 0.3703 | -613.0 | -550.4 | |
| 0 | 4 | 0 | 2 | -10.97 | 173.17 | -12.92 | 138.26 | 0.3311 | -610.0 | -520.8 | |
| 0 | 4 | 0 | 2 | -9.35 | 172.88 | -13.21 | 134.10 | 0.3154 | -847.0 | -700.9 | |
| 0 | 6 | 0 | 3 | -11.18 | 172.52 | -13.57 | 137.29 | 0.3408 | -318.0 | -483.0 | |
| 0 | 5 | 0 | 3 | -11.63 | 171.81 | -14.28 | 136.74 | 0.3541 | -844.0 | -603.1 | |
| 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. | |