| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 81.06 | 445.35 | 41.30 | 226.86 | -16.36 | 12.74 | 6.54 | 207.82 | 0.2343 | 1048.7 | 423.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.36 | 263.94 | 20.61 | 134.74 | -16.59 | 13.53 | 7.33 | 210.24 | 0.2438 | 1428.5 | 467.5 | |
| 4.50 | -1.00 | 2.30 | -1.00 | -16.72 | 12.85 | 6.65 | 207.65 | 0.2401 | 1119.4 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -15.97 | 12.61 | 6.41 | 208.35 | 0.2270 | 942.0 | 759.2 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -15.79 | 12.48 | 6.28 | 208.27 | 0.2233 | 937.0 | 807.8 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -16.21 | 12.41 | 6.20 | 207.06 | 0.2289 | 552.0 | 433.2 | |
| 0.00 | 7.48 | 0.00 | 3.79 | -15.34 | 12.29 | 6.08 | 208.52 | 0.2150 | 351.0 | 401.4 | |
| 0.00 | 1.61 | 0.00 | 0.82 | -14.83 | 11.94 | 5.73 | 208.30 | 0.2045 | -686.0 | -618.8 | |
| 36.20 | 160.61 | 18.39 | 81.58 | -16.09 | 11.78 | 5.58 | 204.94 | 0.2225 | 1337.9 | 414.3 | |
| 0.00 | 0.93 | 0.00 | 0.47 | -14.86 | 11.63 | 5.42 | 206.94 | 0.2026 | 791.0 | 612.9 | |
| 0.00 | 2.21 | 0.00 | 1.12 | -14.47 | 11.44 | 5.23 | 207.03 | 0.1952 | -825.0 | -741.5 | |
| 0.00 | 1.10 | 0.00 | 0.56 | -16.50 | 8.13 | 1.92 | 188.82 | 0.2109 | -1050.0 | -874.8 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -15.72 | 7.51 | 1.31 | 186.45 | 0.1962 | -953.0 | -787.7 | |
| 0.00 | 0.93 | 0.00 | 0.47 | -16.05 | 7.39 | 1.18 | 185.68 | 0.2017 | -929.0 | -646.9 | |
| 0.00 | 1.10 | 0.00 | 0.55 | -12.48 | 4.18 | -2.03 | 165.98 | 0.1434 | -904.0 | -677.6 | |
| 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. | |