| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.49 | 23.92 | 5.18 | 20.57 | -15.33 | 39.19 | -52.92 | 109.61 | 0.8180 | 118.7 | -27.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.65 | 10.34 | 2.11 | 8.24 | -16.32 | 42.87 | -49.25 | 111.76 | 0.7851 | 771.3 | 535.8 | |
| 3.84 | -1.00 | 3.07 | -1.00 | -16.48 | 42.77 | -49.35 | 111.92 | 0.7865 | 711.1 | 999999 | |
| 0.00 | 0.68 | 0.00 | 0.57 | -16.07 | 40.48 | -51.64 | 110.75 | 0.8080 | 502.0 | 398.9 | |
| 0.00 | 1.11 | 0.00 | 0.94 | -15.22 | 39.79 | -52.33 | 109.54 | 0.8127 | 474.0 | 368.5 | |
| 0.00 | 1.11 | 0.00 | 0.97 | -15.82 | 38.49 | -53.63 | 109.93 | 0.8263 | 328.0 | 279.0 | |
| 0.00 | 0.68 | 0.00 | 0.60 | -13.98 | 38.02 | -54.10 | 107.63 | 0.8270 | 315.0 | 273.9 | |
| 0.00 | 1.88 | 0.00 | 1.68 | -15.34 | 37.46 | -54.65 | 109.11 | 0.8347 | 377.0 | 344.2 | |
| 0.00 | 0.85 | 0.00 | 0.78 | -14.64 | 36.38 | -55.73 | 108.06 | 0.8432 | -613.0 | -580.2 | |
| 0.00 | 0.94 | 0.00 | 0.87 | -14.55 | 36.14 | -55.97 | 107.90 | 0.8451 | -541.0 | -534.0 | |
| 0.00 | 0.94 | 0.00 | 0.87 | -14.40 | 35.98 | -56.13 | 107.69 | 0.8463 | -662.0 | -585.6 | |
| 0.00 | 0.26 | 0.00 | 0.24 | -14.56 | 35.92 | -56.19 | 107.86 | 0.8471 | -438.0 | -431.3 | |
| 0.00 | 2.14 | 0.00 | 2.02 | -15.30 | 35.34 | -56.78 | 108.60 | 0.8535 | -577.0 | -452.4 | |
| 0.00 | 1.37 | 0.00 | 1.28 | -13.13 | 35.35 | -56.76 | 106.08 | 0.8499 | -443.0 | -387.4 | |
| 0.00 | 1.62 | 0.00 | 1.51 | -12.76 | 35.43 | -56.69 | 105.67 | 0.8487 | -493.0 | -473.9 | |
| 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. | |