| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.35 | 60.62 | 15.42 | 42.05 | -13.08 | 118.87 | -40.01 | 116.43 | 0.7015 | 313.0 | 126.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.98 | 34.93 | 4.09 | 23.88 | -13.15 | 119.80 | -39.09 | 117.04 | 0.6917 | 793.7 | 382.8 | |
| 10.91 | -1.00 | 7.44 | -1.00 | -12.86 | 119.85 | -39.03 | 116.69 | 0.6896 | 978.5 | 999999 | |
| 1.06 | -1.00 | 0.73 | -1.00 | -13.45 | 119.62 | -39.27 | 117.33 | 0.6953 | 404.1 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.79 | -13.84 | 119.10 | -39.79 | 117.53 | 0.7031 | 353.0 | 218.0 | |
| 0.88 | 2.55 | 0.61 | 1.76 | -13.08 | 119.09 | -39.79 | 116.54 | 0.6992 | 574.5 | 308.5 | |
| 0.00 | 2.38 | 0.00 | 1.63 | -11.54 | 118.89 | -39.99 | 114.40 | 0.6938 | 669.0 | 594.9 | |
| 0.00 | 3.43 | 0.00 | 2.39 | -13.12 | 118.48 | -40.41 | 116.25 | 0.7062 | -162.0 | -54.4 | |
| 0.00 | 0.70 | 0.00 | 0.49 | -11.73 | 118.54 | -40.35 | 114.46 | 0.6987 | 487.0 | 411.8 | |
| 0.62 | 2.55 | 0.44 | 1.81 | -14.31 | 117.94 | -40.95 | 117.47 | 0.7181 | -699.7 | -615.2 | |
| 0.00 | 1.76 | 0.00 | 1.24 | -13.34 | 118.11 | -40.78 | 116.33 | 0.7114 | -213.0 | -39.8 | |
| 0.00 | 1.06 | 0.00 | 0.74 | -11.94 | 117.85 | -41.03 | 114.37 | 0.7074 | 439.0 | 410.6 | |
| 0.00 | 0.97 | 0.00 | 0.69 | -13.66 | 117.34 | -41.55 | 116.31 | 0.7213 | 440.0 | 397.1 | |
| 0.00 | 1.50 | 0.00 | 1.07 | -13.89 | 117.16 | -41.72 | 116.52 | 0.7243 | -305.0 | -413.7 | |
| 0.00 | 0.97 | 0.00 | 0.70 | -13.63 | 116.05 | -42.84 | 115.60 | 0.7350 | -541.0 | -437.8 | |
| 2.46 | 4.31 | 1.79 | 3.13 | -13.41 | 116.06 | -42.83 | 115.32 | 0.7339 | -707.3 | -570.4 | |
| 0.00 | 1.14 | 0.00 | 0.83 | -13.03 | 116.06 | -42.83 | 114.84 | 0.7322 | -658.0 | -599.5 | |
| 0.44 | 1.23 | 0.32 | 0.90 | -13.23 | 115.89 | -43.00 | 115.01 | 0.7349 | -625.6 | -541.7 | |
| 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. | |