| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.02 | 216.56 | 26.92 | 116.43 | -11.71 | 178.48 | -13.87 | 142.97 | 0.3902 | 465.5 | 270.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.37 | 184.49 | 1.27 | 98.75 | -11.93 | 179.48 | -12.87 | 145.19 | 0.3834 | 867.1 | 394.3 | |
| 1.23 | -1.00 | 0.66 | -1.00 | -11.90 | 179.23 | -13.12 | 144.63 | 0.3854 | 784.4 | 999999 | |
| 34.46 | -1.00 | 18.45 | -1.00 | -11.53 | 179.15 | -13.20 | 143.89 | 0.3812 | 1213.6 | 999999 | |
| 0.88 | -1.00 | 0.47 | -1.00 | -11.09 | 179.11 | -13.24 | 143.10 | 0.3759 | 907.0 | 999999 | |
| 0.53 | -1.00 | 0.28 | -1.00 | -11.38 | 178.75 | -13.60 | 142.83 | 0.3831 | 708.2 | 999999 | |
| 1.23 | 3.34 | 0.66 | 1.80 | -12.14 | 178.49 | -13.86 | 143.51 | 0.3954 | 671.4 | 511.4 | |
| 1.23 | 5.98 | 0.67 | 3.26 | -12.67 | 176.87 | -15.48 | 141.25 | 0.4177 | -830.5 | -777.2 | |
| 2.99 | -7.00 | 1.63 | -7.00 | -12.80 | 176.61 | -15.74 | 140.99 | 0.4220 | -894.4 | 999999 | |
| 0.00 | 1.23 | 0.00 | 0.67 | -13.03 | 176.53 | -15.82 | 141.19 | 0.4255 | -707.0 | -625.1 | |
| 0.00 | 0.70 | 0.00 | 0.39 | -12.12 | 174.31 | -18.04 | 136.04 | 0.4380 | -710.0 | -672.0 | |
| 0.00 | 3.60 | 0.00 | 2.01 | -14.20 | 173.95 | -18.39 | 138.68 | 0.4653 | -580.0 | -526.1 | |
| 2.11 | 7.73 | 1.17 | 4.27 | -12.08 | 173.67 | -18.68 | 134.97 | 0.4446 | -998.3 | -669.4 | |
| 2.99 | 4.04 | 1.66 | 2.24 | -12.56 | 173.57 | -18.78 | 135.59 | 0.4509 | -925.9 | -728.6 | |
| 0.00 | 1.32 | 0.00 | 0.74 | -13.43 | 173.37 | -18.98 | 136.63 | 0.4626 | -822.0 | -632.3 | |
| 0.00 | 1.67 | 0.00 | 0.93 | -13.08 | 173.36 | -18.99 | 136.09 | 0.4588 | -872.0 | -727.1 | |
| 0.00 | 1.23 | 0.00 | 0.68 | -12.70 | 173.33 | -19.02 | 135.44 | 0.4550 | -760.0 | -614.5 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -11.85 | 172.22 | -20.13 | 132.47 | 0.4584 | -803.0 | -651.4 | |
| 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. | |