| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.07 | 101.57 | 15.57 | 83.14 | -8.92 | 247.75 | 52.95 | 262.75 | 0.7959 | 322.5 | 220.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.60 | 71.61 | 1.37 | 60.95 | -8.88 | 249.83 | 55.04 | 262.82 | 0.8183 | 232.8 | 247.9 | |
| 9.04 | -1.00 | 7.69 | -1.00 | -8.85 | 249.51 | 54.71 | 262.86 | 0.8150 | 683.2 | 999999 | |
| 3.37 | -1.00 | 2.84 | -1.00 | -8.75 | 249.12 | 54.32 | 262.98 | 0.8111 | 856.7 | 999999 | |
| 0.00 | 1.42 | 0.00 | 1.19 | -8.37 | 248.93 | 54.14 | 263.45 | 0.8092 | 290.0 | 292.0 | |
| 0.00 | 0.71 | 0.00 | 0.59 | -8.73 | 248.59 | 53.79 | 263.01 | 0.8057 | 654.0 | 551.1 | |
| 0.00 | 0.62 | 0.00 | 0.51 | -8.80 | 248.09 | 53.29 | 262.92 | 0.8006 | 258.0 | 341.9 | |
| 0.00 | 1.60 | 0.00 | 1.21 | -10.42 | 244.44 | 49.64 | 260.76 | 0.7616 | -661.0 | -569.6 | |
| 1.51 | 3.10 | 1.14 | 2.34 | -10.11 | 244.09 | 49.29 | 261.15 | 0.7575 | -637.2 | -515.7 | |
| 0.00 | 1.24 | 0.00 | 0.93 | -9.85 | 243.89 | 49.10 | 261.49 | 0.7553 | -506.0 | -379.6 | |
| 0.00 | 1.24 | 0.00 | 0.91 | -8.61 | 242.51 | 47.72 | 263.12 | 0.7391 | 754.0 | 623.9 | |
| 0.00 | 1.33 | 0.00 | 0.97 | -8.22 | 242.40 | 47.61 | 263.65 | 0.7378 | 644.0 | 574.5 | |
| 0.00 | 9.39 | 0.00 | 6.89 | -9.18 | 242.52 | 47.72 | 262.34 | 0.7393 | 588.0 | 656.0 | |
| 0.89 | 4.61 | 0.64 | 3.31 | -9.29 | 241.37 | 46.57 | 262.16 | 0.7258 | -652.8 | -483.2 | |
| 2.66 | 4.70 | 1.89 | 3.34 | -8.56 | 240.85 | 46.05 | 263.15 | 0.7194 | -677.7 | -546.6 | |
| 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. | |