| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.63 | 0.00 | 11.76 | -18.38 | 50.07 | -24.38 | 127.09 | 0.4909 | 481.4 | 406.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.70 | 0.00 | 2.03 | -15.80 | 53.22 | -21.23 | 125.72 | 0.4309 | 620.0 | 607.6 | |
| 0.00 | 1.17 | 0.00 | 0.64 | -15.14 | 53.12 | -21.32 | 124.30 | 0.4266 | 739.0 | 622.9 | |
| 0.00 | 2.07 | 0.00 | 1.13 | -14.92 | 53.11 | -21.33 | 123.84 | 0.4250 | 801.0 | 613.3 | |
| 0.00 | 1.08 | 0.00 | 0.60 | -18.32 | 52.50 | -21.95 | 129.55 | 0.4620 | 786.0 | 620.6 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -19.33 | 51.94 | -22.51 | 130.63 | 0.4779 | 855.0 | 729.6 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -19.46 | 51.89 | -22.56 | 130.78 | 0.4797 | 640.0 | 571.6 | |
| 0.00 | 1.17 | 0.00 | 0.66 | -18.98 | 51.61 | -22.84 | 129.64 | 0.4786 | 705.0 | 564.1 | |
| 0.00 | 2.89 | 0.00 | 1.64 | -19.99 | 50.96 | -23.48 | 130.61 | 0.4953 | 684.0 | 483.9 | |
| 0.00 | 1.17 | 0.00 | 0.66 | -18.27 | 51.15 | -23.29 | 127.91 | 0.4779 | 617.0 | 425.0 | |
| 0.00 | 0.54 | 0.00 | 0.31 | -19.42 | 50.95 | -23.50 | 129.64 | 0.4903 | 653.0 | 441.2 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -19.35 | 50.57 | -23.88 | 129.11 | 0.4941 | 308.0 | 306.0 | |
| 0.00 | 1.53 | 0.00 | 0.94 | -20.32 | 43.27 | -31.18 | 124.04 | 0.5880 | 669.0 | 575.3 | |
| 0.00 | 1.71 | 0.00 | 1.06 | -21.70 | 42.52 | -31.93 | 125.52 | 0.6059 | -712.0 | -538.1 | |
| 0.00 | 0.90 | 0.00 | 0.56 | -20.24 | 41.92 | -32.53 | 122.93 | 0.6034 | -626.0 | -543.9 | |
| 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. | |